The galaxy presents as a centrally concentrated spheroid with a smooth, featureless appearance. The central region exhibits a yellowish-orange hue, suggesting a population of older, evolved stars. Moving outward from the core, the color transitions to a bluer tone. The morphology appears elliptical, with a predominantly rounded shape. No distinct spiral arms, bars, or other significant structural features are discernible within the galaxy's disk. There is no evidence of any major mergers or significant tidal disturbances affecting the galaxy's overall structure. The galaxy has a slightly diffuse halo.
