NGC 5445
NGC 5445 is a lenticular galaxy in the constellation Canes Venatici about 181 million ly from Earth. It spans roughly 82,000 ly, about 82% of our Milky Way's width. It is receding from us at about 3,900 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 181 million ly from home, you are seeing NGC 5445 as it looked roughly 181 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 5440Spiral8.0 million ly
apartNGC 5444Elliptical8.1 million ly
apartNGC 5533Spiral8.5 million ly
apartNGC 5399Barred spiral12 million ly
apartNGC 5614Spiral13 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).