The galaxy presents a generally elliptical morphology, appearing neither perfectly spherical nor significantly elongated. It exhibits a relatively smooth texture overall, with no immediately obvious spiral arm structures or prominent dust lanes. The central bulge region is bright and concentrated, suggesting a high stellar density. Surrounding the bulge is a less luminous, more diffuse halo or disk component. There is a slight hint of a possible tidal feature or minor disturbance, but further data would be required to confirm this interaction. The galaxy displays a bluer hue overall, particularly within the outer regions.
