The galaxy presents as an elliptical morphology, characterized by a smooth, centrally concentrated luminosity profile. The overall color is yellowish-orange, suggesting a stellar population dominated by older, redder stars and a relative paucity of ongoing star formation. The galaxy exhibits a slight elongation, approximating a prolate spheroid. There is a subtle asymmetry in the outer regions of the galaxy's halo, indicating a possible interaction or minor disturbance. The central bulge is prominent and appears well-defined. No obvious spiral arms or disk-like features are discernible. The overall appearance suggests a relatively evolved system.
