The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates into a more diffuse halo. Color gradients are subtle, with a yellowish-white core transitioning to a fainter, slightly bluish-green outer region. No distinct spiral arms or dust lanes are visible. The galaxy appears largely undisturbed, without obvious signs of tidal interactions or major mergers. Its overall morphology suggests a system dominated by older stellar populations, with a low rate of current star formation. The galaxy's round shape indicates its dynamics are primarily supported by random motions.
