NGC 5292

NGC 5292 is a spiral galaxy in the constellation Centaurus about 206 million ly from Earth. It spans roughly 140,000 ly, about the width of our Milky Way. It is receding from us at about 4,487 km/s.

Because its light is 206 million ly from home, you are seeing NGC 5292 as it looked roughly 206 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).