The galaxy appears as a slightly inclined disk galaxy, approximately 3.8 kpc in radius. The galaxy exhibits a faint central bulge and a disk with some structural features. The color index suggests the presence of both older stellar populations in the bulge, and bluer, younger populations in the disk. There may be minor signs of disturbance present, but the overall structure seems relatively unperturbed. Star formation appears to be ongoing, but at a relatively low rate. The galaxy is likely of intermediate mass.
