NGC 1495
NGC 1495 is a spiral galaxy in the constellation Horologium about 60 million ly from Earth. It spans roughly 39,000 ly, about 39% of our Milky Way's width. It is receding from us at about 1,245 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 60 million ly from home, you are seeing NGC 1495 as it looked roughly 60 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 1448Spiral5.8 million ly
apartNGC 1483Barred spiral6.6 million ly
apartNGC 1494Spiral8.3 million ly
apartIC 2035Elliptical8.8 million ly
apartNGC 1436Spiral9.6 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).