This galaxy appears to be a relatively smooth, elliptical galaxy. Its overall shape is generally round. The central region exhibits a concentrated, bright core, which decreases in intensity radially outward. There is little evidence of spiral arms or a prominent disk structure. The color profile suggests a relatively old stellar population, particularly within the core region, with a gradual shift to slightly bluer hues in the outer regions. There appears to be no significant major disturbances or signs of an ongoing or recent major merger event. Minor disturbances are possible, but not clearly evident. The light distribution indicates a single, centralized galactic structure.
