The galaxy presents as a relatively smooth, centrally concentrated object with an overall elliptical morphology. There is a distinct color gradient visible, with the central region exhibiting a yellowish-white hue, indicative of an older stellar population. The outer regions show a subtle shift towards redder tones, potentially indicating a mix of intermediate-age stars or dust obscuration. No distinct spiral arms or bar structures are discernible. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions with other galaxies, though there are subtle signs of minor disturbances. The overall structure suggests the galaxy is primarily supported by random stellar motions. The estimated size appears to be moderate, neither exceptionally large nor particularly compact.
