IC 167
IC 167 is a spiral galaxy in the constellation Aries about 137 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 2,960 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 137 million ly from home, you are seeing IC 167 as it looked roughly 137 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.
apartIC 1730Spiral870,000 ly
apartNGC 680Elliptical3.8 million ly
apartNGC 678Barred spiral5.2 million ly
apartNGC 674Spiral8.1 million ly
apartIC 163Barred spiral8.5 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).