The galaxy presents with an elliptical morphology, though exhibiting some disk-like characteristics. The light distribution is centrally concentrated, appearing brightest at the core, and gradually decreases toward the outer edges. The core region exhibits a yellowish-white hue, suggesting a population of older stars. There is a subtle hint of bluer light in the outer regions, possibly indicating some ongoing star formation, albeit at a low rate. Overall, the galaxy appears relatively smooth in texture, with no obvious signs of major mergers or significant tidal disturbances. However, subtle asymmetries in the outer regions cannot be ruled out, hinting at possible minor interactions.
