The galaxy presents as a largely featureless elliptical galaxy with a smooth light profile, exhibiting a nearly circular morphology. A slight color gradient is observable, with a central region appearing more red, indicative of an older stellar population. There is no discernible spiral arm structure or dust lane obscuration. The overall appearance suggests a well-relaxed system, possibly having undergone past merger events but exhibiting no current signs of major tidal disruption. The lack of strong blue color suggests a relatively low rate of ongoing star formation.
