The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that appears luminous in the green-yellow wavelengths. The galaxy displays a generally round morphology, with a slight deviation suggesting a possible minor disturbance or interaction. There is no prominent disk structure, and spiral arms are not visible. Color gradients suggest that the central regions are likely dominated by older stellar populations compared to the faint outer edges of the galaxy. There are no obvious signs of major mergers or significant tidal features.
