The galaxy presents as a largely featureless elliptical type. It has a smooth, centrally concentrated luminosity profile, indicative of an older stellar population. The color gradient shows a redder core transitioning to a slightly bluer halo. No distinct spiral arms or bar structures are discernible. There are no signs of ongoing major mergers, although some minor disturbances cannot be ruled out based on the overall smoothness. The galaxy has a roughly circular appearance.
