NGC 5612
NGC 5612 is a spiral galaxy in the constellation Apus about 129 million ly from Earth. It spans roughly 73,000 ly, about 73% of our Milky Way's width. It is receding from us at about 2,699 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 129 million ly from home, you are seeing NGC 5612 as it looked roughly 129 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 4522Barred spiral8.9 million ly
apartIC 4377Lenticular9.2 million ly
apartIC 4545Spiral10 million ly
apartNGC 5967ASpiral11 million ly
apartNGC 5967Spiral13 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).