The galaxy presents as a generally smooth object with a centrally concentrated brightness profile. It appears mostly elliptical in shape. The core region exhibits a yellowish-white hue, suggesting an older stellar population, while the outer regions present a bluer color, possibly indicative of more recent star formation. There are no apparent spiral arms or a prominent galactic disk. A minor disturbance or asymmetry in the structure is potentially visible, but the system appears to be generally unperturbed. The galaxy appears somewhat round rather than elongated. There is no obvious evidence of an ongoing major merger event.