The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. The core appears bright and gradually fades into the surrounding halo. There is a general lack of distinct features such as spiral arms or prominent dust lanes. A slight asymmetry is observable, with a hint of a possible minor disturbance or interaction. The object appears rounded, though there may be a very subtle elongation. The color gradient seems minimal, indicating a fairly uniform stellar population across the observed wavelengths. There are no significant signs of active star formation regions visible.
