The galaxy exhibits a primarily smooth, elliptical morphology. The core is intensely bright, indicating a high concentration of stars. The light profile appears centrally concentrated, diminishing gradually toward the outer regions. The galaxy shows a slight elongation. The color gradient suggests a population of older stars. No spiral arm structure or dust lanes are apparent. The object appears relatively undisturbed, with no signs of recent merger activity. The overall color is moderately red, consistent with an older stellar population. The observed structure is consistent with a high Sersic index, indicative of an elliptical galaxy.
