The galaxy presents a largely smooth morphology, suggestive of an elliptical or lenticular type. The galaxy exhibits a centrally concentrated light profile, with a bright, yellowish core that gradually fades outwards. A subtle disk-like feature may be present, but it is not well-defined. The color gradients suggest a population of older stars dominating the central regions, with potentially younger, bluer populations residing in the outer parts of the galaxy. There is no obvious sign of significant ongoing star formation or merger activity, though minor disturbances cannot be ruled out. The galaxy appears relatively isolated, with no close companions readily apparent in this field of view.
