The galaxy presents as a moderately luminous, relatively smooth elliptical-type galaxy. It exhibits a dominant, centrally concentrated bulge that transitions smoothly into a diffuse outer halo. The central region appears to be yellowish-white suggesting a population of older stars. No prominent dust lanes or spiral arm structures are discernible. Overall, the morphology suggests a galaxy that is largely undisturbed, with a lack of ongoing major star formation. Its shape is generally rounded, but with a slight elongation along one axis. There is a possible minor disturbance of some kind, though the image quality limits more definitive conclusions.
