NGC 7167
NGC 7167 is a barred spiral galaxy in the constellation Aquarius about 120 million ly from Earth. It spans roughly 64,000 ly, about 64% of our Milky Way's width. It is receding from us at about 2,583 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 120 million ly from home, you are seeing NGC 7167 as it looked roughly 120 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 7247Barred spiral9.7 million ly
apartIC 1438Spiral11 million ly
apartNGC 7208Lenticular11 million ly
apartNGC 7183Lenticular12 million ly
apartNGC 7204ABarred spiral14 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).