NGC 5410
NGC 5410 is a spiral galaxy in the constellation Canes Venatici about 174 million ly from Earth. It spans roughly 58,000 ly, about 58% of our Milky Way's width. It is receding from us at about 3,738 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 174 million ly from home, you are seeing NGC 5410 as it looked roughly 174 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 5341Barred spiral11 million ly
apartNGC 5401Spiral15 million ly
apartNGC 5395Spiral16 million ly
apartNGC 5394Barred spiral16 million ly
apartNGC 5325Spiral18 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).