The galaxy appears as a centrally concentrated, elliptical-like object with a smooth, featureless morphology. The galaxy exhibits a subtly elongated shape, appearing more "in-between" round and cigar shaped, lacking any distinct spiral arms or a bar structure. A slight color gradient is observed, with the core region exhibiting a somewhat bluer hue compared to the outer regions. This suggests the presence of a younger stellar population in the center. No significant signs of ongoing mergers or tidal disturbances are apparent, indicating it is a relatively undisturbed system, although minor disturbances cannot be ruled out. Overall, the galaxy appears to be a quiescent system with a relatively low star formation rate and a substantial stellar mass.
