The galaxy presents as a centrally concentrated object, elliptical in appearance. It exhibits a smooth light distribution, with no obvious spiral arm structures or distinct features visible in this image. The color gradient suggests an older stellar population, trending towards redder hues in the central region and somewhat bluer colors extending to the outer halo. There is little evidence of active star formation, based on the lack of blue color concentration within the galactic structure. The overall morphology is consistent with an elliptical galaxy that has undergone minimal recent merger activity, presenting a more relaxed structure.
