NGC 1177
NGC 1177 is an elliptical galaxy in the constellation Perseus about 260 million ly from Earth. It spans roughly 45,000 ly, about 45% of our Milky Way's width. It is receding from us at about 5,584 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 260 million ly from home, you are seeing NGC 1177 as it looked roughly 260 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 310Lenticular12 million ly
apartIC 300Elliptical12 million ly
apartIC 265Elliptical13 million ly
apartIC 262Lenticular13 million ly
apartNGC 1260Lenticular14 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).