The galaxy presents as a primarily smooth, centrally concentrated object. It has an elliptical morphology, appearing largely rounded in shape. Some minor irregularities and disturbances can be observed, but its general structure is well-defined and undisturbed, appearing as if it has undergone minimal recent merging events. The galaxy displays a yellowish hue, suggesting a stellar population dominated by older, evolved stars and relatively low ongoing star formation. The outer regions of the galaxy gradually fade into the background, with no prominent spiral arms or distinct features immediately visible. The galaxy is relatively compact in size, with a distinct core surrounded by fainter regions.