The galaxy presents as a luminous, relatively compact object. It appears primarily elliptical in shape, exhibiting a smooth light distribution with a concentrated central bulge that transitions outwards into a diffuse halo. The core is a bright yellow color, and the halo has areas of light orange. There is little evidence of spiral arms or significant dust lanes; the general morphology suggests an older stellar population and a relatively low star formation rate for its estimated mass. A slight irregularity in the halo may indicate an ongoing minor merger event or some past gravitational disturbance.
