The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge dominates the overall structure, displaying a bright, nearly spherical core. Moving outward from the core, the light gradually diminishes, creating a diffuse halo. There is a slight bluing of the galaxy's halo, suggestive of ongoing, albeit low, star formation activity. No clear spiral arm structures or prominent dust lanes are visible within the resolution of the image. There are no immediately apparent signs of any recent major merger events or strong tidal disturbances, only possible minor disturbance. The galaxy is well-defined and appears isolated.
