The galaxy presents as a moderately bright, elliptical structure with a discernible central bulge that appears luminous and concentrated. The disk component is visible, displaying a somewhat flattened shape. There is a subtle color gradient, the central bulge exhibiting a yellow-white hue while the outer regions appear slightly bluer, possibly indicative of younger stellar populations within the disk. The galaxy does not display strong evidence of ongoing major merger activity, although there is a slight asymmetry.
