James Webb Space Telescope posted a photo:

Webb took a high resolution look at a supermassive black hole, the one at the center of the Circinus Galaxy, changing the way scientists think about how black holes interact with the matter around them.
While black holes are themselves invisible, they can actually be a source of bright light if matter like gas and dust gets a bit too close. A donut-shaped ring can form around the black hole, called a torus. Matter from the torus’ inner walls can form a thinner (accretion) disk that spirals inward to the black hole itself, similar to a whirlpool of water swirling around a drain. Through friction, the matter in this disk gets really hot and bright. Some black holes also launch jets of matter into space, which is what happens when some of this matter falling toward the black hole gets sped up to nearly the speed of light and thrown off it. The resulting brightness (combined with starlight from Circinus) can make it hard to resolve details through the glare. The torus causes different problems because it is dense and obscures visible light, so it is a challenge to see through.
The combination of Webb seeing infrared light (which pierces through dust and gas) and being extra powerful is giving scientists data they were missing. Before Webb, models made by scientists using existing data of Circinus, suggested that most of the brightness of a black hole is due to those powerful jets. Webb reverses that thinking though, showing that 87% of the infrared light from hot dust in Circinus comes from the areas closest to the black hole, while less than 1% come from the outflowing jets.
This, of course, is only one black hole amongst billions in the universe, so understanding black holes as a, well, whole, is not quite so simple. However, astronomers now have a tested technique for better investigating other black holes.
Read more: go.nasa.gov/3NaFazp
Image description: An artist’s illustration showing the center of the Circinus galaxy, including its supermassive black hole, dusty torus, and superheated jets of matter. The center of supermassive black hole, slightly left of center, is bright white. Two slim, bright green jets of matter shoot out from the black hole at 1 o’clock and 7 o’clock, and hit the edges of the frame. A donut-shaped, orangish-pinkish ring of dust and gas, called a torus, surrounds the black hole. The disk is clumpy closer to the center and more diffuse at the edges. The torus, tilted at the same angle as the jets, is brighter and whiter closer to the black hole than at the edges. The words "Artist’s Concept" are in the lower right corner.
Credits: NASA, ESA, CSA, Ralf Crawford (STScI)