NGC 690
NGC 690 is a spiral galaxy in the constellation Cetus about 243 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 5,231 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 243 million ly from home, you are seeing NGC 690 as it looked roughly 243 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 682Elliptical19 million ly
apartNGC 594Barred spiral19 million ly
apartIC 160Elliptical23 million ly
apartNGC 593Lenticular24 million ly
apartIC 129Lenticular25 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).