The galaxy presents as a largely smooth, elliptical-like structure. Its light profile exhibits a strong central concentration, becoming less dense toward the outer edges. The core appears bright, suggesting a high stellar density or potential active galactic nucleus. The overall color of the galaxy is yellowish-white, which could indicate an older stellar population with a lower rate of ongoing star formation. Faint hints of reddish hues can be observed at the periphery of the galaxy. The object shows a fairly rounded morphology. There are no visible signs of spiral arms or significant dust lanes. There is no indication of major tidal disturbances or ongoing merger activity.
