The galaxy presents as a relatively bright, centrally concentrated object. It exhibits a generally smooth, elliptical morphology with no readily discernible spiral arm structure. The core region displays a yellow-white hue, suggesting a population of older stars. Fainter, bluer light emanates from the outer regions of the galaxy, potentially indicating some ongoing star formation. The object's roundness suggests it's likely an elliptical galaxy that is not observed at a significant angle. There is some slight evidence of minor disturbances in the galaxy's shape.
