NGC 3659
NGC 3659 is a spiral galaxy in the constellation Leo about 60 million ly from Earth. It spans roughly 34,000 ly, about 34% of our Milky Way's width. It is receding from us at about 1,234 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 60 million ly from home, you are seeing NGC 3659 as it looked roughly 60 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 3592Spiral2.4 million ly
apartNGC 3608Elliptical4.8 million ly
apartNGC 3522Elliptical5.1 million ly
apartNGC 3596Spiral5.7 million ly
apartNGC 3684Barred spiral5.7 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).