The galaxy presents as a fairly luminous, elliptical structure. It exhibits a generally smooth morphology with a concentrated central bulge. The galaxy's color profile suggests a population of older stars, as indicated by the yellowish hue, especially concentrated within the bulge. There is a subtle elongation visible, presenting an intermediate shape between round and cigar-shaped. Faint extensions or tidal features are not readily apparent, and the overall structure suggests it is not currently undergoing a major merger event. The relatively smooth appearance and color profile indicate a system with a low star formation rate.
