The galaxy presents as a largely smooth, centrally concentrated structure. The light is dominated by a yellowish hue, potentially indicating an older stellar population. The shape appears generally elliptical, with the majority of its profile concentrated towards the center, then gradually fading out to the edges. There is a very small percentage of the light emanating from the outer edges, which indicates a very subtle disc shape. There are no evident spiral arms or significant dust lanes, which points towards the conclusion that it is either a lenticular or an elliptical galaxy type. The core shows a high degree of concentration, with no signs of disturbances or merging events.