The galaxy appears as a centrally concentrated, elliptical-like system. The light profile is smooth and diffuse, exhibiting a radial color gradient. The core region presents with a yellowish-white hue, indicative of an older stellar population. This color transitions to a bluer, albeit subtle, halo in the outer regions of the galaxy. The overall morphology suggests minimal ongoing star formation. There may be evidence of minor disturbances or interactions due to slight asymmetries in the outer halo, though the system appears largely relaxed and unperturbed. The galaxy exhibits a moderate size. It presents a lack of spiral arm structures and dust lanes, further supporting classification as an early-type galaxy.
