| NGC 3786 | |
| Image Scale: | 1.5 |
| Epoch: | J2000 |
| Z: | 0.008883 |
| Type: | (R')SA(rs)a |
| Appmag V: | 13.74 |
| Appmag B: | 14.62 |
| Names: | , Mark 744 |
NGC 3786 is an intermediate spiral galaxy located 32.95e6pc away in the northern constellation of Ursa Major. It was discovered by English astronomer John Herschel on April 10, 1831. This object appears to form a close pair with its peculiar neighbor to the north, NGC 3788. They show some indications of interaction, such as minor distortion of the disk or tidal features.
The morphological classification of this galaxy is (R')SA(rs)a, indicating a spiral galaxy (SA) with an outer ring (R'), transitional inner ring (rs), and tightly wound spiral arms (a). The galactic plane is inclined at an angle of to the line of sight from the Earth. A mini-bar structure appears in the circumnuclear region. It is a type 1.8 Seyfert galaxy, with a detectable X-ray emission that is being partially absorbed by warm, dusty material along the line of sight. The active galactic nucleus of this galaxy is driven by a supermassive black hole with an estimated mass of . An outburst from the core was observed in 1996 and a mid-infrared flare in 2022.
Type Ic supernova SN 1999bu was detected from an image taken April 16, 1999. It was magnitude 17.5 and was located at an offset west and south of the galactic nucleus of NGC 3786. A possible progenitor to this core collapse supernova event was identified in 2003 from archival images. A second supernova, SN 2004bd, was discovered April 7, 2004. This was a type Ia supernova located west and south of the nucleus.