The galaxy presents as a centrally concentrated object with a smooth, featureless appearance. The light profile suggests a dominant spheroidal component. Its overall shape is elliptical, appearing somewhat elongated, but not significantly so, with its roundness more in between round and cigar shaped. There is no strong evidence of spiral arms, dust lanes, or other distinct morphological features. The galaxy exhibits a color gradient, with a whiter, more luminous core transitioning to a bluer, fainter outer halo, suggesting a population of older stars concentrated towards the center and younger stars in the outer regions. There is no apparent signs of ongoing or recent major merger activity.
