The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. Its overall colour index suggests a population of older stars, contributing to the observed reddish-orange hue. There are no immediately apparent signs of spiral arms or significant dust lanes. The galaxy appears largely undisturbed, with no major morphological disturbances indicative of recent or ongoing merger activity, though subtle irregularities can not be ruled out with certainty given the image resolution. The object's roundness appears close to circular. It seems to have a relatively quiescent star formation rate. The galaxy has substantial mass. 
