The galaxy presents as a single, largely featureless object. It has a smooth, elliptical morphology, appearing almost perfectly round. The color profile suggests a generally evolved stellar population, with a yellowish-orange core indicative of older stars and a lower rate of star formation in the central region. The outer regions show a slightly bluer tint, possibly indicating the presence of younger stars, but the overall star formation rate appears relatively low. There is no apparent spiral structure or bar. There is no indication of any ongoing major merger events or significant tidal disturbances. It exhibits a concentrated central bulge with a diffuse halo.
