NGC 191
NGC 191 is a spiral galaxy in the constellation Cetus about 283 million ly from Earth. It spans roughly 82,000 ly, about 82% of our Milky Way's width. The light reaching us tonight left it about 283 million years ago.
Illustration from its catalogued shape, not a photograph
Because its light is 283 million ly from home, you are seeing NGC 191 as it looked roughly 283 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.
apartIC 48Lenticular7.0 million ly
apartIC 50Elliptical9.2 million ly
apartNGC 163Elliptical9.8 million ly
apartNGC 165Barred spiral11 million ly
apartNGC 155Lenticular12 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).