The galaxy appears as a centrally concentrated spheroid with a smooth morphology. The light profile suggests a lack of significant spiral arm structure or prominent dust lanes. The color gradient indicates a possible population of older stars dominating the central region, displaying a yellowish hue. Based on the shape, the object likely exhibits characteristics of an elliptical galaxy. Some signs of a minor disturbance are present in the outer regions, with some fuzziness in the halo.&#x20;
