The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears more luminous than the surrounding regions. There is no obvious spiral arm structure visible. The color profile suggests a population of older stars, indicated by the yellowish-red hue of the central bulge, while the outer regions appear slightly bluer, hinting at a small presence of younger stellar populations or ongoing, but weak, star formation. The morphology appears generally undisturbed.
