NGC 1530
NGC 1530 is a barred spiral galaxy in the constellation Camelopardalis about 115 million ly from Earth. It spans roughly 61,000 ly, about 61% of our Milky Way's width. It is receding from us at about 2,506 km/s.
Illustration from its catalogued shape, not a photograph
Because its light is 115 million ly from home, you are seeing NGC 1530 as it looked roughly 115 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.
apartIC 334Spiral6.5 million ly
apartNGC 1343Spiral14 million ly
apartNGC 1184Lenticular15 million ly
apartNGC 2336Barred spiral23 million ly
apartNGC 2268Barred spiral24 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).