The galaxy presents a predominantly smooth and elliptical morphology. It exhibits a bright, concentrated central bulge that appears yellow-white. The light diffuses outwards, fading into a fainter, bluish halo with a slightly flattened disk. The galaxy appears undisturbed with no signs of major mergers or tidal tails. There is a hint of subtle structure with a faint, thin disk and minimal dust lanes that are nearly edge-on. The red color of the central bulge suggests older stellar populations, with the bluer halo indicating the presence of younger, hotter stars in a low level of star formation.
