The galaxy appears as an elliptical structure, exhibiting a smooth, largely featureless morphology. Its color profile suggests a dominant population of older stars, with a redder hue in the central regions. The galaxy displays a well-defined core, with a gradual decrease in luminosity towards its outer edges. There is little evidence of active star formation, consistent with a more evolved system. There is a slight indication of a potential minor disturbance, but the overall structure appears relatively undisturbed. The shape is predominantly round, with a marginal deviation towards a more spheroidal form.