NGC 3455
NGC 3455 is a spiral galaxy in the constellation Leo about 52 million ly from Earth. It spans roughly 34,000 ly, about 34% of our Milky Way's width. It is receding from us at about 1,113 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 52 million ly from home, you are seeing NGC 3455 as it looked roughly 52 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 3443Spiral820,000 ly
apartNGC 3457Elliptical1.7 million ly
apartNGC 3447BIrregular1.8 million ly
apartNGC 3501Spiral2.0 million ly
apartNGC 3447ASpiral2.5 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).