This galaxy presents as an edge-on spiral system. A prominent central bulge dominates the galaxy's morphology, displaying a smooth, rounded structure. The disk appears thin and elongated, exhibiting a defined dust lane that bisects the bulge. Faint spiral arm structures are tentatively discernible extending away from the central bulge, but are not very well defined. There is no obvious major distortion in the overall shape, however there are indications of a minor disturbance. Its red color suggests an older stellar population. The estimated size appears to be moderate, neither a dwarf nor a giant galaxy. Based on its general morphology, the galaxy is likely to have ceased actively forming stars long ago.
