The galaxy presents as a fairly smooth, elliptical object. It exhibits a concentrated central bulge that diminishes gradually toward its outer edges. The galaxy appears somewhat flattened. There is a subtle color gradient, with the core region appearing slightly yellower than the outer regions, potentially indicating a higher concentration of older stars in the center. No distinct spiral arms or prominent dust lanes are visible. The overall structure suggests a system dominated by an older stellar population with a relatively low ongoing star formation rate.
