The galaxy exhibits a generally elliptical morphology, though it does not appear perfectly smooth. There is a bright, concentrated central bulge, surrounded by a fainter, more diffuse halo. The galaxy displays a noticeable disk-like structure, oriented at a moderate inclination relative to our line of sight. The color gradient suggests a population of older stars dominating the central regions, with potentially younger, bluer stars sparsely distributed throughout the disk. Slight disturbances or asymmetries are possibly present in the outer regions of the disk. The object appears fairly isolated with no immediate interacting companions visible in this field.
