| NGC 4088 | |
|---|---|
Composite image of NGC 4088 | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 12h 05m 34.2s |
| Declination | +50° 32′ 21″ |
| Redshift | 0.002524 |
| Heliocentric radial velocity | 757 ± 1 km/s (470.4 ± 0.6 mi/s) |
| Distance | 51.5 ± 4.5 Mly (15,800 ± 1,400 kpc) |
| Apparent magnitude (V) | 11.2 |
| Characteristics | |
| Type | SAB(rs)bc |
| Apparent size (V) | 5.8′ × 2.2′ |
| Other designations | |
| UGC 7081, PGC 38302, Arp 18, VV 357 | |
NGC 4088 is a barred spiral galaxy in the constellation Ursa Major. The galaxy forms a physical pair with NGC 4085, which is located 11′ away.

NGC 4088 is a grand design spiral galaxy. This means that the spiral arms in the galaxy's disk are sharply defined. In visible light, one of the spiral arms appears to have a disconnected segment. Halton Arp included this galaxy in the Atlas of Peculiar Galaxies as one of several examples where this phenomenon occurs.
NGC 4088 and NGC 4085 are members of the M109 Group, a group of galaxies located in the constellation Ursa Major. This large group contains between 41 and 58 galaxies, including the spiral galaxy M109.
Three supernovae have been observed in NGC 4088: