NGC 5131
NGC 5131 is a spiral galaxy in the constellation Canes Venatici about 319 million ly from Earth. It spans roughly 42,000 ly, about 42% of our Milky Way's width. It is receding from us at about 6,851 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 319 million ly from home, you are seeing NGC 5131 as it looked roughly 319 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 4238Spiral6.7 million ly
apartIC 4227Barred spiral8.1 million ly
apartIC 4242Barred spiral14 million ly
apartNGC 5052Lenticular17 million ly
apartNGC 5187Barred spiral17 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).