NGC 5440
NGC 5440 is a spiral galaxy in the constellation Canes Venatici about 174 million ly from Earth. It spans roughly 140,000 ly, about the width of our Milky Way. It is receding from us at about 3,754 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 174 million ly from home, you are seeing NGC 5440 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 5401Spiral5.5 million ly
apartNGC 5445Lenticular8.0 million ly
apartNGC 5533Spiral10 million ly
apartNGC 5351Barred spiral11 million ly
apartNGC 5341Barred spiral12 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).