The galaxy presents as a relatively smooth and centrally concentrated object. Its overall shape is somewhat elliptical, appearing more in between circular and elongated. The galaxy exhibits a gradual increase in light intensity towards its center, where the brightest region resides. There is no obvious sign of spiral arms or a prominent disk structure. Faint hints of disturbances around the main body, possibly indicating a minor interaction or past merger event, are not exluded. The color profile seems to be dominated by yellowish-red hues, suggesting a population of older stars and a relatively low star formation rate.
