The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions gradually into a diffuse halo. The overall color profile suggests an older stellar population, with a yellow-red hue dominating the central region and some bluer tinges appearing within the outer regions. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy appears relatively undisturbed, showing no obvious signs of ongoing major mergers or tidal interactions. The shape is generally round. Overall, the galaxy is indicative of a relatively quiescent, evolved system.
