The galaxy appears to be an elliptical galaxy, exhibiting a smooth and largely featureless morphology. It presents with a bright, concentrated central bulge, indicating a high stellar density in the core region. The overall shape is moderately elongated, deviating slightly from a perfect circular form. The color gradient suggests an aging stellar population, with a yellowish hue dominating the central regions transitioning to a bluer periphery. There is no visible evidence of spiral arms, dust lanes, or ongoing star formation within the observable extent of the galaxy. The outer regions appear diffuse and fade gradually into the background, showing no clear signs of tidal interactions or recent merger events.
