The galaxy presents as a centrally concentrated, luminous spheroid. It exhibits a smooth and featureless morphology, lacking apparent spiral arms or a prominent disk structure. The color gradient suggests a population of older stars, with the central region displaying a yellowish-white hue, indicative of evolved stellar populations. The outer regions gradually fade into a bluer tint. The overall shape is elliptical, with a slight elongation, but generally appears rounded. There is no obvious sign of significant dust lanes or recent major merger events. It shows a smooth, elliptical distribution of light that gradually decreases in intensity from the bright core outward.
