The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated morphology with a gradual decrease in luminosity towards its outer regions. The core displays a yellowish hue, potentially indicating an older stellar population. There are no prominent spiral arms or distinct features readily visible. There is a slight asymmetry, which may suggest minor disturbances. A faint, elongated structure extending from the main body could be indicative of tidal interactions or a minor merger event. Overall, the galaxy's appearance suggests a significant mass concentration and relatively low levels of ongoing star formation.
