The galaxy presents as a somewhat elliptical structure with a notable central bulge. Its overall color is predominantly yellow-orange, suggesting an older stellar population and lower rates of ongoing star formation. There are hints of a disk structure extending from the central bulge, although it is not sharply defined and appears relatively smooth. The galaxy exhibits a moderately elongated shape; it is neither perfectly spherical nor highly flattened. There is no obvious indication of a major merger event or strong tidal disturbances. Subtle asymmetry in the outer regions suggests a possible minor interaction or internal disturbance. The lack of prominent blue regions indicates a limited presence of young, hot stars.
