The galaxy presents a generally elliptical morphology, with a smooth, diffuse light distribution. The core is brighter than the outskirts and slightly elongated. While there is no distinct spiral arm structure visible, the overall shape suggests it may be an early-type spiral. Color gradients are subtle, with a slightly bluer hue toward the outer regions, suggestive of some ongoing, albeit weak, star formation. No prominent dust lanes or other features of asymmetry are immediately apparent, though some minor disturbances may be present due to the galaxy's asymmetric features.
