NGC 6890
NGC 6890 is a barred spiral galaxy in the constellation Sagittarius about 112 million ly from Earth. It spans roughly 52,000 ly, about 52% of our Milky Way's width. It is receding from us at about 2,471 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 112 million ly from home, you are seeing NGC 6890 as it looked roughly 112 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 6861ESpiral11 million ly
apartNGC 6861CLenticular13 million ly
apartNGC 6909Elliptical16 million ly
apartIC 5011Lenticular18 million ly
apartNGC 6870Spiral18 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).