The galaxy presents a primarily elliptical morphology, exhibiting a centrally concentrated bulge that gradually fades outward. The light distribution appears relatively smooth with no well-defined spiral arm structures immediately evident. The galaxy exhibits a moderate blue color, suggesting the presence of a young stellar population and ongoing star formation activity, even though the overall appearance is more typical of an elliptical galaxy. Some minor disturbances appear to be present, indicating that the galaxy may have undergone a minor merger in the past. There are no clear signs of a current, major merger event.
