The galaxy appears as a single, luminous object with a smooth, elliptical morphology. A bright, concentrated core region dominates the galaxy's visual structure, suggesting a high stellar density towards the center. The light profile transitions smoothly from the core to a more diffuse halo, with no apparent spiral arm structure or distinct features, the galaxy appears to have no on-going major merging event. Color gradients suggest a stellar population that is old and redder in the central regions. The galaxy is not perfectly spherical; it has a slight elongation. Overall, the galaxy presents as a relatively undisturbed system with minimal recent star formation activity.