NGC 4197
NGC 4197 is a spiral galaxy in the constellation Virgo about 96 million ly from Earth. It spans roughly 79,000 ly, about 79% of our Milky Way's width. It is receding from us at about 2,049 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 96 million ly from home, you are seeing NGC 4197 as it looked roughly 96 million years ago. The photons left before that much of history had passed, and are only now reaching us. This distance is estimated from the galaxy's redshift, so the lookback time is approximate.
apartNGC 4269Lenticular2.3 million ly
apartNGC 4268Lenticular3.6 million ly
apartNGC 4234Spiral3.7 million ly
apartNGC 4287Barred spiral4.5 million ly
apartNGC 4255Lenticular5.7 million ly
apart
Source: structural data (position, morphology, brightness, redshift) from OpenNGC (CC BY-SA). Recession velocity from RC3 (de Vaucouleurs et al. 1991, via NASA/HEASARC, public domain). Distance computed by gravityfinder from redshift via Hubble's law (H0 = 70 km/s/Mpc).