The galaxy presents as a centrally concentrated object, with a smooth, generally elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars and relatively low dust content in the central region. There is a subtle color gradient, transitioning to a slightly redder and less intense outer halo. No distinct spiral arms or other detailed features are discernible, indicating a likely classification as an elliptical galaxy. The overall appearance suggests a relatively evolved system, possibly undergoing limited current star formation activity. There is no apparent strong tidal disruption or merging activity.
