This galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge, characterized by a yellow-orange hue, suggesting an older stellar population. The outer regions display a more diffuse and bluish coloration, possibly indicating the presence of younger stars or ongoing, though subdued, star formation. The galaxy's overall shape is somewhat elongated but predominantly rounded. There is no immediately obvious evidence of strong spiral arm structure or major disturbances suggestive of a recent significant merger event. The galaxy's size is relatively compact. There may be hints of a faint, extended halo surrounding the main body, but its presence is not definitively discernible from the available image. Overall, the galaxy presents as a mature, relatively quiescent system.
