This galaxy presents as a centrally concentrated, ellipsoidal system with a smooth light profile. There is little to no discernible disk structure. The galaxy's overall color appears to be dominated by redder wavelengths, indicating an older stellar population and/or significant dust obscuration. The shape appears close to elliptical, though there is some elongation. There is no obvious evidence of tidal features, strong dust lanes, or ongoing major mergers. The galaxy shows a slight color gradient, with the central regions appearing more yellowish-orange, suggesting a higher concentration of older stars toward the core. There are no signs of distinct spiral arms.
