NGC 677
NGC 677 is an elliptical galaxy in the constellation Aries about 236 million ly from Earth. It spans roughly 120,000 ly, about the width of our Milky Way. It is receding from us at about 5,100 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 236 million ly from home, you are seeing NGC 677 as it looked roughly 236 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 673Spiral7.8 million ly
apartNGC 683Barred spiral9.9 million ly
apartIC 162Lenticular10 million ly
apartIC 156Spiral18 million ly
apartIC 161Lenticular18 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).