The galaxy exhibits a morphology that appears to be undergoing a significant interaction or merger. The primary body displays a generally smooth, spheroidal structure with a concentrated, luminous core, indicative of an evolved stellar population. The overall color of the core is reddish-yellow.

Connected to the primary spheroid is a fainter, more diffuse structure. This feature appears elongated and less symmetrical. It shows a bluish tinge.

The presence of both a smooth, redder component and a more disturbed, bluer component suggests a complex system, possibly representing an ongoing merger. The smooth component likely represents the pre-existing, more massive galaxy, while the disturbed component may be a smaller galaxy that is being disrupted by tidal forces. Alternatively, the disturbed component may represent tidal debris or newly formed stars triggered by the interaction.

The system's redshift indicates that it is located at a considerable distance. This is further evidenced by the faintness of its apparent magnitude. At this distance, it would be expected to be quite massive. The low star formation rate suggests that the interaction is in a later stage.
