NGC 1796

NGC 1796 is a barred spiral galaxy in the constellation Dorado about 47 million ly from Earth. It spans roughly 27,000 ly, about 27% of our Milky Way's width. It is receding from us at about 966 km/s.

Because its light is 47 million ly from home, you are seeing NGC 1796 as it looked roughly 47 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.

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).