NGC 4189
NGC 4189 is a spiral galaxy in the constellation Coma Berenices about 98 million ly from Earth. It spans roughly 63,000 ly, about 63% of our Milky Way's width. It is receding from us at about 1,995 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 98 million ly from home, you are seeing NGC 4189 as it looked roughly 98 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 4152Spiral5.1 million ly
apartIC 769Barred spiral5.4 million ly
apartNGC 4352Lenticular5.8 million ly
apartIC 3074Barred spiral6.1 million ly
apartIC 3220Elliptical6.1 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).