This galaxy presents as a centrally concentrated object with a smooth morphology. The light distribution indicates a likely spheroidal shape, though not perfectly round. The core region exhibits a yellowish-white hue suggesting a population of older stars. A faint blueish halo or disk-like structure is discernible surrounding the central bulge, indicating the presence of some younger stars or ongoing star formation within a disk component. No major disturbances or tidal features are apparent, hinting at a relatively undisturbed evolutionary history. The size appears moderate, neither exceptionally large nor particularly compact. There are no prominent spiral arms or bar features visible. Overall, it has characteristics of a late-type galaxy with intermediate mass.
