NGC 1219
NGC 1219 is a spiral galaxy in the constellation Cetus about 285 million ly from Earth. It spans roughly 98,000 ly, about the width of our Milky Way. It is receding from us at about 6,101 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 285 million ly from home, you are seeing NGC 1219 as it looked roughly 285 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 1305Elliptical28 million ly
apartNGC 1101Lenticular28 million ly
apartNGC 1323Lenticular32 million ly
apartNGC 1095Barred spiral32 million ly
apartNGC 1322Elliptical33 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).