NGC 1889
NGC 1889 is an elliptical galaxy in the constellation Lepus about 116 million ly from Earth. It spans roughly 21,000 ly, about 21% of our Milky Way's width. It is receding from us at about 2,482 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 116 million ly from home, you are seeing NGC 1889 as it looked roughly 116 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 1784Spiral11 million ly
apartNGC 1888Barred spiral12 million ly
apartNGC 1924Barred spiral13 million ly
apartIC 407Spiral19 million ly
apartNGC 2110Elliptical19 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).