The galaxy presents as a generally smooth, elliptical morphology. The light profile appears centrally concentrated, exhibiting a high degree of circular symmetry. There is little to no discernible disk structure or spiral arm features visible. The galaxy's color appears to be redder in the central regions, transitioning towards a slightly bluer hue in the outer regions. This suggests the presence of a stellar population gradient, with older, redder stars dominating the core and a younger, bluer stellar population populating the outskirts. No obvious signs of recent or ongoing major mergers or tidal disturbances are apparent. The overall appearance is indicative of an evolved system.
