The galaxy presents as a relatively smooth, lenticular or early-type spiral morphology. It exhibits a bright, concentrated central bulge that dominates the overall luminosity profile. The isophotes appear generally elliptical, trending toward a circular shape. A faint, diffuse disk is discernible extending outwards from the bulge. The disk shows some evidence of subtle, disturbed features or a lack of strong spiral arm structure. Patches of bluer light are present within the disk, suggestive of possible ongoing star formation, though at a low rate. Overall color indices indicate a population dominated by older, redder stars. There is no apparent evidence of a major ongoing merger or significant tidal interactions.
