NGC 1596
NGC 1596 is a lenticular galaxy in the constellation Dorado about 70 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 1,465 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 70 million ly from home, you are seeing NGC 1596 as it looked roughly 70 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 1602Barred spiral3.6 million ly
apartNGC 1581Elliptical5.1 million ly
apartIC 2049Spiral5.1 million ly
apartIC 2058Spiral5.3 million ly
apartNGC 1703Barred spiral7.3 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).