The galaxy presents as a single, centrally concentrated object. A smooth, spheroidal morphology is evident. The core exhibits a yellowish-white hue, suggesting an older stellar population. The surrounding halo displays a bluer tint, possibly indicating the presence of younger, hotter stars. The overall shape is largely elliptical, appearing quite round. There is no clear indication of spiral arms or a defined disk structure. No major disturbances or mergers are apparent in this image, though minor interactions may be occurring.
