The galaxy presents as a relatively smooth, elliptical object. Its color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue concentrated towards the center. The outer regions display a slight decrease in intensity. The galaxy exhibits a somewhat elongated morphology, deviating slightly from a perfectly circular shape. There appears to be little to no evidence of spiral arms or significant dust lanes, furthering the conclusion of an elliptical classification. There is no apparent major interaction or merging event occurring with this galaxy.
