NGC 1989
NGC 1989 is an elliptical galaxy in the constellation Columba about 501 million ly from Earth. It spans roughly 250,000 ly, about 2.5 times the width of our Milky Way. It is receding from us at about 10,782 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 501 million ly from home, you are seeing NGC 1989 as it looked roughly 501 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 408Lenticular60 million ly
apartIC 411Lenticular76 million ly
apartIC 2125Lenticular83 million ly
apartIC 2119Barred spiral120 million ly
apartNGC 1692Lenticular120 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).