The galaxy presents a complex morphology, displaying characteristics of both a smooth spheroidal component and features indicative of a possible disk. A dominant, centrally concentrated bulge exhibits a yellowish hue, suggesting a population of older stars. Extending outwards from this central region, fainter, somewhat bluer structures are visible. These may represent a more flattened disk component with ongoing star formation. There is no discernable spiral structure within the disk, with a somewhat flocculent appearance. The overall shape of the galaxy is somewhere between round and elliptical, without clear signs of a major ongoing merger event, but some indications of minor disturbances.
