The galaxy presents as a centrally concentrated, elliptical system with a smooth, largely featureless morphology. It exhibits a near-perfect circular symmetry. A gradual decrease in luminosity emanates outwards from a bright core. Color gradients indicate a yellowish-white hue in the central regions, transitioning to a slightly bluer color in the outer halo. There is no discernible spiral arm structure or evidence of significant dust lanes. The overall appearance suggests a relatively evolved galaxy, potentially with a high fraction of older stellar populations. There are no obvious signs of tidal disturbances or ongoing merger activity.
