The galaxy presents as an elliptical or lenticular structure, exhibiting a smooth, centrally concentrated morphology. There is a distinct lack of resolved spiral arms or prominent dust lanes, suggesting an older stellar population. The core region is bright and appears roughly spheroidal, diminishing gradually in intensity towards the outer regions. There is a slight elongation, indicating it is somewhere in between round and cigar-shaped. Faint features suggest the possibility of some minor disturbances. Overall, the object appears to be an evolved galaxy, likely with a relatively low rate of star formation. The primary color gradient shifts from yellow-white at the core, toward red-orange in the outer halo.