The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated, bright central bulge that transitions into a more diffuse halo. The core appears yellowish-white, suggesting a population of older stars. The outer regions of the galaxy show a subtle color gradient, with a slightly bluer hue, potentially indicating areas of ongoing, though subdued, star formation activity. The overall morphology is largely undisturbed, with no prominent tidal features or signs of a major merger event. The galaxy appears generally rounded. There are no discernible spiral arms or a prominent disk structure.
