NGC 2990
NGC 2990 is a spiral galaxy in the constellation Sextans about 144 million ly from Earth. It spans roughly 39,000 ly, about 39% of our Milky Way's width. It is receding from us at about 3,150 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 144 million ly from home, you are seeing NGC 2990 as it looked roughly 144 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 2914Barred spiral14 million ly
apartNGC 2911Lenticular15 million ly
apartNGC 2939Barred spiral16 million ly
apartNGC 2872Elliptical21 million ly
apartNGC 2873Spiral21 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).