NGC 118
NGC 118 is an elliptical galaxy in the constellation Cetus about 521 million ly from Earth. It spans roughly 120,000 ly, about the width of our Milky Way. It is receding from us at about 11,250 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 521 million ly from home, you are seeing NGC 118 as it looked roughly 521 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 141Lenticular72 million ly
apartNGC 138Spiral74 million ly
apartIC 1565Elliptical85 million ly
apartIC 1569Lenticular86 million ly
apartNGC 139Barred spiral89 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).