The galaxy presents as a somewhat symmetrical, moderately concentrated light distribution. It appears as a spheroidal galaxy, appearing primarily smooth in texture. The central region exhibits a slightly brighter and more condensed core with a faint, diffuse halo extending outwards. There is a very faint indication of a possible very small disk structure at the very center of the galaxy. The color profile suggests a predominantly older stellar population. Evidence for ongoing or recent major mergers is absent, though there may be hints of minor tidal disturbances or interactions. Overall, the galaxy appears relatively undisturbed.