The galaxy presents as a centrally concentrated object with a primarily smooth morphology. It exhibits a generally elliptical appearance, displaying a high degree of roundness with no discernible bar structure. There is a very slight suggestion of a faint outer halo, but this is minimal. No distinct spiral arm features are visible within the observable light. Overall, this galaxy shows morphological properties consistent with an early-type galaxy. There is no clear indication of ongoing major merger activity, though the possibility of minor interactions or disturbances cannot be ruled out. The color suggests a redder stellar population, consistent with an older, passively evolving system.
