The galaxy appears as a centrally concentrated object with a smooth, diffuse light distribution. It exhibits a generally elliptical morphology, showing no obvious spiral arm structures or prominent dust lanes within the visible spectrum. The light from the central region is bright and fades gradually into the outer regions, without any clear defined edges. There is a slight blue tint in its outer regions, and its center appears yellow. The overall impression is of a relatively quiescent system, potentially an elliptical galaxy or a lenticular galaxy viewed at a sufficient distance such that any disk structure is not easily discernible. There are no apparent signs of recent major merger activity, although a slight disturbance might be present within the galactic halo.
