The galaxy appears as a centrally concentrated object with a smooth, diffuse light distribution. It presents a nearly circular morphology, with no readily apparent spiral arm structures or a pronounced disk component discernible in this image. The light profile suggests a significant spheroidal component. The galaxy exhibits a yellowish hue, indicative of a relatively older stellar population and a lower rate of ongoing star formation. There is no evidence of any major mergers or tidal disturbances affecting its structure.
