The galaxy presents as a well-defined elliptical structure with a smooth, concentrated central bulge. A diffuse halo surrounds the brighter central region. There is a slight flattening of the overall shape, suggesting it is not perfectly spherical but rather somewhat oblate. The color distribution indicates an older stellar population, with a yellowish-red hue dominating the central regions and a subtle blueish tint in the outer halo. There is no visible evidence of distinct spiral arms or significant dust lanes. Overall, the galaxy appears relatively undisturbed, showing no signs of major ongoing mergers or tidal interactions, with, at most, minor disturbances present.
