NGC 789
NGC 789 is a barred spiral galaxy in the constellation Triangulum about 244 million ly from Earth. It spans roughly 49,000 ly, about 49% of our Milky Way's width. It is receding from us at about 5,116 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 244 million ly from home, you are seeing NGC 789 as it looked roughly 244 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 200Barred spiral4.9 million ly
apartNGC 804Lenticular5.8 million ly
apartNGC 750Elliptical6.6 million ly
apartNGC 798Elliptical9.4 million ly
apartNGC 778Lenticular9.4 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).