This galaxy exhibits a generally elliptical morphology, though there appears to be a disk structure. A pronounced central bulge dominates the galaxy's luminosity profile. The disk component shows some evidence of spiral arm structure, however, this is somewhat ill-defined. The light distribution is centrally concentrated, with a relatively smooth transition from the bulge to the disk. The outer regions of the disk are less luminous. There appears to be moderate inclination with respect to our line of sight, obscuring some of the disk features. Overall, the galaxy presents as a disk galaxy with a substantial bulge component, displaying characteristics intermediate to a spiral and elliptical morphology. There does not appear to be any major sign of disturbance due to merging. A weak bar feature might be present.
