The galaxy presents as a smooth, elongated elliptical shape. It exhibits a concentrated central bulge that gradually diffuses outwards into a fainter halo. The color gradient transitions from a yellowish-orange core to a bluer periphery, potentially indicative of varying stellar populations. A significant proportion of the light appears to originate from older stars within the galactic center, while a small portion of younger, bluer stars may be present in the outer regions. The morphology suggests minimal tidal disruption or ongoing merger activity, exhibiting a well-defined structure with no obvious signs of disturbance. There is a subtle hint of a disk, although it is not clearly defined. The galaxy displays a moderate luminosity. Overall, the characteristics align with a mature galaxy undergoing relatively little current star formation.
