The galaxy presents a morphology suggestive of a spiral or lenticular type, exhibiting a centrally concentrated bulge region that gradually diffuses outward. The light distribution indicates a relatively smooth structure. The central bulge exhibits a bright, whitish-yellow hue, possibly indicating a population of older stars. Extending outwards from the bulge, a fainter disk is observed with a bluer tint, potentially caused by the presence of younger stars and ongoing star formation. There may be some minor distortions in the morphology, suggesting past or ongoing gravitational interactions. The overall light profile appears somewhat elliptical, with a defined major axis.
