The galaxy presents a smooth, elliptical morphology. A bright, concentrated core dominates the central region, surrounded by a more diffuse halo that gradually fades into the background. The galaxy appears relatively undisturbed, lacking any obvious signs of spiral arms or tidal features. Its overall color suggests a relatively old stellar population, with a lack of prominent blue regions that would indicate recent star formation. The shape is elongated, hinting at possible rotation or an ongoing merging event, though no clear second nucleus is visible. The surface brightness profile appears to follow a de Vaucouleurs law, indicative of an elliptical galaxy.
