NGC 2470
NGC 2470 is a spiral galaxy in the constellation Canis Minor about 191 million ly from Earth. It spans roughly 110,000 ly, about the width of our Milky Way. It is receding from us at about 4,114 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 191 million ly from home, you are seeing NGC 2470 as it looked roughly 191 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 2510Lenticular18 million ly
apartNGC 2508Elliptical19 million ly
apartNGC 2561Barred spiral21 million ly
apartNGC 2526Spiral24 million ly
apartIC 503Spiral24 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).