The galaxy appears as a moderately bright, elliptical or lenticular system. It exhibits a smooth, centrally concentrated light profile, with a gradual decrease in brightness towards the outer edges. The core region presents a yellowish-white hue, potentially indicative of an older stellar population dominating the nucleus. Moving outwards from the center, there's a slight hint of bluer tones. The galaxy's overall structure seems relatively undisturbed. Evidence suggests this system is undergoing only weak star formation. Given these observations, the galaxy is likely a mature system.
