The galaxy presents as a centrally concentrated, smooth, elliptical-like structure. It exhibits a radial color gradient, transitioning from a yellowish core to a bluer halo. The central region appears relatively featureless. The overall shape is largely spheroidal with only a slight deviation from perfect circularity. There are no apparent signs of strong tidal interactions or major mergers, however, there may be some minor distortions or irregularities in the outer regions of the galaxy. Star formation appears to be relatively low, with a dominantly older stellar population as indicated by the redder core.
