This galaxy presents as a largely featureless elliptical galaxy with a smooth, concentrated light profile. The central bulge appears quite luminous with a yellowish hue, potentially indicating an older stellar population dominating this region. There is a slight extension of the light distribution beyond the central bulge. Based on the morphology, star formation appears suppressed. No dust lanes or spiral arm structures are discernible, which would align with a largely quiescent system that has undergone or is undergoing processes that result in the lack of star formation. There may be some minor interaction with another galaxy occurring.