NGC 1024
NGC 1024 is a spiral galaxy in the constellation Aries about 163 million ly from Earth. It spans roughly 140,000 ly, about the width of our Milky Way. It is receding from us at about 3,521 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 163 million ly from home, you are seeing NGC 1024 as it looked roughly 163 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 1029Lenticular3.8 million ly
apartNGC 1107Lenticular11 million ly
apartIC 267Barred spiral12 million ly
apartNGC 1134Barred spiral14 million ly
apartIC 1790Spiral19 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).