NGC 1961

NGC 1961 is a spiral galaxy in the constellation Camelopardalis about 182 million ly from Earth. It spans roughly 230,000 ly, about 2.3 times the width of our Milky Way. It is receding from us at about 3,983 km/s.

Because its light is 182 million ly from home, you are seeing NGC 1961 as it looked roughly 182 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.

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).