The galaxy presents as a predominantly smooth, elliptical structure. The overall color profile suggests an older stellar population, with a concentration of light towards the central bulge. There is a subtle, flattened disk-like appearance, though features are not sharply defined. Little active star formation is evident from its colors. The galaxy exhibits a generally round morphology, lacking any significant tidal tails, bridges, or other indicators of a major merger event. There is a slight asymmetry, suggesting the possibility of a past minor interaction or ongoing accretion event. The system appears relatively undisturbed.