The galaxy presents a smooth, elliptical morphology. The light distribution appears concentrated towards the center, exhibiting a high degree of circular symmetry. The color index indicates a population of older stars dominating the light emission, with minimal evidence of ongoing star formation. There are no obvious signs of spiral arms or a prominent disk structure, which suggests it is likely an elliptical galaxy. There are no signs of tidal tails or other obvious disturbances that would indicate a recent merger event. Overall, the galaxy appears relatively undisturbed and quiescent.
