The galaxy presents as a primarily smooth, centrally concentrated object with a slight elongation. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a more bluish-white, possibly indicating the presence of younger stars. A subtle, disk-like structure may be present, but it is not highly pronounced. There is minimal evidence of strong star formation, and no apparent major disturbances or ongoing mergers. The overall morphology leans towards an elliptical or lenticular classification, with a moderate size. The galaxy appears relatively undisturbed and evolved.
