The galaxy presents as a somewhat smooth, centrally concentrated object with a slight elongation in its overall shape. The core region appears bright and yellowish-white, suggesting an older stellar population. A faint, diffuse blue halo surrounds the central region, potentially indicative of recent star formation. No prominent spiral arms or strong dust lanes are visible. The overall morphology suggests a galaxy transitioning between a spiral and elliptical type, or possibly a lenticular galaxy. There is no readily apparent indication of any major ongoing merger activity.
