The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology with a moderate degree of roundness. There is a distinct central bulge region displaying a yellowish hue, suggesting an older stellar population is dominant in this area. The outer regions of the galaxy show a gradual decline in surface brightness, with hints of a faint disk structure. Overall, the galaxy appears undisturbed, without major signs of ongoing mergers or tidal interactions, although some subtle distortions cannot be ruled out. The general colour suggests a somewhat moderate level of star formation, with older stars dominating the central region.
