The galaxy presents as a centrally concentrated, smooth object. It exhibits an elliptical morphology with a moderate axis ratio, appearing somewhat elongated but not highly flattened. The light profile suggests a dominant bulge component.

A subtle color gradient is discernible. The central region displays a yellowish-white hue, possibly indicating a population of older stars. The outer regions show a slight bluer tint, suggesting the presence of some younger stellar populations or ongoing, albeit low-level, star formation activity. No prominent spiral arms or distinct features such as dust lanes or star clusters are immediately apparent. There seems to be a minor disturbance of the smooth appearance, however there are no major signs of merger activity.
