The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. It exhibits a moderate axis ratio, suggesting a flattened spheroidal shape, but not a highly elongated structure. The color gradient is subtle, with the core appearing slightly more yellow-white, implying a population of older stars, while the outer regions possess a somewhat bluer hue, possibly indicating the presence of younger stellar populations or low-level star formation activity. There is no obvious dust lane or spiral arm structure visible, which is consistent with an early-type galaxy. Overall, the galaxy appears to be a relatively undisturbed system with a well-defined structure.
