The galaxy appears as a moderately sized elliptical system, displaying a relatively smooth and concentrated light profile. There is some indication of a faint, diffuse halo extending beyond the main body of the galaxy, but the resolution limits a detailed analysis of its structure. The overall color is generally redder, suggestive of an older stellar population and a lower rate of ongoing star formation. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. It presents an elliptical morphology that is neither perfectly spherical nor highly elongated. 