NGC 5289
NGC 5289 is a spiral galaxy in the constellation Canes Venatici about 116 million ly from Earth. It spans roughly 79,000 ly, about 79% of our Milky Way's width. It is receding from us at about 2,446 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 116 million ly from home, you are seeing NGC 5289 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 5313Spiral4.6 million ly
apartNGC 5297Spiral4.8 million ly
apartIC 4336Barred spiral4.9 million ly
apartNGC 5346Spiral5.0 million ly
apartNGC 5350Barred spiral5.1 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).