NGC 3495
NGC 3495 is a spiral galaxy in the constellation Leo about 52 million ly from Earth. It spans roughly 71,000 ly, about 71% of our Milky Way's width. It is receding from us at about 1,086 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 52 million ly from home, you are seeing NGC 3495 as it looked roughly 52 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 692Elliptical8.3 million ly
apartIC 2828Irregular8.3 million ly
apartNGC 3666Barred spiral9.0 million ly
apartNGC 3705Spiral9.6 million ly
apartIC 2767Spiral9.9 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).