NGC 4231
NGC 4231 is a lenticular galaxy in the constellation Canes Venatici about 346 million ly from Earth. It spans roughly 78,000 ly, about 78% of our Milky Way's width. It is receding from us at about 7,418 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 346 million ly from home, you are seeing NGC 4231 as it looked roughly 346 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 4226Barred spiral8.4 million ly
apartNGC 4392Lenticular15 million ly
apartNGC 4288ALenticular21 million ly
apartNGC 4109Spiral33 million ly
apartIC 731Barred spiral37 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).