NGC 1022
NGC 1022 is a barred spiral galaxy in the constellation Cetus about 69 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 1,498 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 69 million ly from home, you are seeing NGC 1022 as it looked roughly 69 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 963Irregular3.8 million ly
apartNGC 1084Spiral4.0 million ly
apartNGC 988Spiral4.1 million ly
apartNGC 991Spiral4.1 million ly
apartNGC 1042Spiral4.9 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).