The galaxy presents a generally elliptical morphology, with a smooth, centrally concentrated light profile. Its core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The galaxy's outer regions appear fainter and slightly more reddish, potentially indicating the presence of dust or a different stellar population. There are no clear spiral arm structures visible, further supporting the classification as an elliptical galaxy. The overall shape indicates that it is moderately flattened. There is no strong evidence of any recent major merging events or significant tidal disturbances.
