The galaxy presents as a largely smooth, elliptical-like structure with a centrally concentrated luminosity. There is a noticeable colour gradient, shifting from a yellowish-white hue in the core region to a redder shade in the outer regions. The overall shape is somewhat elongated, though not exceptionally so. There is no apparent disk structure. No significant dust lanes or distinct spiral arms are visible. There are no signs of tidal tails or strong morphological disturbances that would indicate a recent major merger event, although there are indications of a minor disturbance. The outskirts of the galaxy appear diffuse and lack well-defined edges. Overall, the galaxy presents as a passively evolving system with a considerable stellar mass.
