NGC 600
NGC 600 is a spiral galaxy in the constellation Cetus about 86 million ly from Earth. It spans roughly 66,000 ly, about 66% of our Milky Way's width. It is receding from us at about 1,867 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 86 million ly from home, you are seeing NGC 600 as it looked roughly 86 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 615Barred spiral790,000 ly
apartNGC 584Elliptical1.1 million ly
apartIC 127Barred spiral1.4 million ly
apartNGC 636Elliptical2.3 million ly
apartNGC 586Spiral3.9 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).