The galaxy exhibits a primarily smooth morphology, suggesting a relatively evolved system. The light distribution is concentrated toward the center, forming a bright, elliptical core. Moving outward from the center, the light intensity gradually decreases. There is some indication of a slight disk-like structure, with hints of features or arms faintly visible in the outer regions. The overall shape is slightly elongated, not perfectly round, with an approximate cigar shaped appearance. No signs of major mergers are apparent, though subtle disturbances may be present, potentially indicative of minor interactions or internal dynamical processes. Color gradients are visible, with the central region appearing more yellow/white, likely indicating an older stellar population, while the outer regions show some blueish tones, suggesting the presence of younger stars.
