This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. Its color is predominantly yellowish-orange, suggesting an older stellar population with fewer young, hot blue stars. The galaxy exhibits a centrally concentrated bulge region which appears round and smooth. There is a slight suggestion of a disk structure, although it lacks prominent spiral arms or distinct features. Some minor disturbances or asymmetries may be present in its outer regions. The galaxy appears to be isolated, with no obvious signs of recent or ongoing major merger activity.
