The black hole is warping spacetime around it in a severe fashion. The innermost (unstable) orbit is called the photon sphere, and light can make several orbits around the hole before either falling in, or going off to infinity. The result is that (depending on the hole’s rotation relative to your point of view) you’re going to see roughly the same image we have today. You’re actually going to see multiple images of the entire hole, stretched around the outer edge, and those images multiplied and distorted again. If you could somehow “stand” by the photon spehere you’d see the back of your own head many many times.
The other factor is that while the event horizon itself is a spheroid, the accretion disk of bright infalling material is not. The horizon is totally black, so it will always look roughly like seeing a disk face-on no matter where you look at it. The accretion disk is a “hoop” that’s stretched and the image is multiplied and distorted by the strong warping of spacetime in the region. As a result you get smeared and repeated views of the entire disk including portion behind the hole in a kind of bent band. Plus the whole thing is subject to strong Doppler beaming hence the bright and dark regions.
The other factor is that while the event horizon itself is a spheroid, the accretion disk of bright infalling material is not. The horizon is totally black, so it will always look roughly like seeing a disk face-on no matter where you look at it. The accretion disk is a “hoop” that’s stretched and the image is multiplied and distorted by the strong warping of spacetime in the region. As a result you get smeared and repeated views of the entire disk including portion behind the hole in a kind of bent band. Plus the whole thing is subject to strong Doppler beaming hence the bright and dark regions.