The galaxy presents a largely smooth, elliptical morphology. A centrally concentrated bulge of older stellar populations is visible, indicated by the yellowish-red color at its core. This core transitions outwards into a more diffuse halo.

There is little evidence of significant spiral arm structure or prominent dust lanes within the galaxy. It exhibits a fairly regular, rounded shape, deviating negligibly from perfect sphericity. No obvious signs of ongoing major mergers or significant tidal disturbances are present. There is a faint blue hint in the surrounding halo, potentially representing a small amount of ongoing or recent star formation. 
