The galaxy presents as a smooth, elliptical morphology. Its color profile indicates a dominant population of older stars, with a yellowish core. The galaxy exhibits a generally low rate of star formation, and the presence of minimal dust lanes is suggested by the smooth appearance. There is little evidence of spiral arm structure or recent mergers. The object's light is centrally concentrated, diminishing smoothly toward its outer regions, indicating an absence of distinct substructures within the galaxy.
