The galaxy presents as a largely featureless, elliptical structure. It exhibits a smooth, centrally concentrated light profile, with a bright core that gradually diminishes in intensity toward the outer edges. The isophotes appear to be nearly circular, showing minimal deviation from a perfect ellipse. Color gradients are subtle, with a slightly yellower hue toward the central region, possibly indicating a higher concentration of older stellar populations. The outer regions appear slightly bluer, which may be due to recent star formation within the disk. There are no prominent dust lanes or spiral arm structures visible. Overall, the galaxy's morphology suggests a relatively evolved system, consistent with classification as an elliptical galaxy.
