The galaxy presents as a relatively smooth, elliptical form. Its core appears bright and concentrated, suggesting a high stellar density. Moving outward from the center, the luminosity gradually decreases, with no distinct spiral arm structures or prominent dust lanes visible. The galaxy exhibits a moderate ellipticity, appearing more oval than circular. There is a slight indication of a possible tidal feature or minor disturbance located on the outer edge of the galaxy, however more data is needed to confirm this. Color suggests a redder, more evolved stellar population.
