The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a notable color gradient present, transitioning from a reddish hue in the galactic center to a greenish-yellowish tinge in the outer regions. The smoothness suggests a lack of significant spiral arm structure or dust lanes. The object appears relatively undisturbed, with no obvious signs of ongoing or recent major merger activity. The round appearance indicates a lack of strong ellipticity. Based on the color profile, there might be some ongoing star formation in the outer regions, as indicated by the greenish-yellowish hue, although the central red color suggests an older stellar population is present.