NGC 3475
NGC 3475 is a spiral galaxy in the constellation Leo about 298 million ly from Earth. It spans roughly 98,000 ly, about the width of our Milky Way. It is receding from us at about 6,350 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 298 million ly from home, you are seeing NGC 3475 as it looked roughly 298 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 3327Barred spiral22 million ly
apartNGC 3615Elliptical28 million ly
apartIC 2590Lenticular30 million ly
apartNGC 3618Spiral31 million ly
apartNGC 3270Spiral32 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).