IC 288
IC 288 is a spiral galaxy in the constellation Perseus about 241 million ly from Earth. It spans roughly 71,000 ly, about 71% of our Milky Way's width. It is receding from us at about 5,094 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 241 million ly from home, you are seeing IC 288 as it looked roughly 241 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 266Lenticular10 million ly
apartIC 294Lenticular10 million ly
apartNGC 1267Elliptical11 million ly
apartIC 300Elliptical11 million ly
apartPerseus ALenticular11 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).