This galaxy presents as a largely featureless elliptical or lenticular system. It exhibits a smooth, centrally concentrated light distribution. There may be some asymmetry present in the outer regions of the galaxy, possibly indicating a minor gravitational disturbance or interaction with a smaller companion. The main body of the galaxy has a roughly round shape, with no prominent bar or spiral arm structures visible. Color gradients suggest a population of older stars, potentially with some ongoing star formation in the central region. There appears to be a relatively red central bulge, surrounded by a bluer disk. Further observations would be helpful to identify whether the disturbance is related to a minor merger or simply tidal effects.
