The galaxy exhibits a complex morphology, appearing to be in a state of interaction or recent merger. A dominant, centrally located component displays a relatively smooth, roundish appearance with a concentrated core. This core is marked by a bluish hue, suggestive of younger stellar populations or active galactic nucleus activity.

Extending outward from this central component is a less defined region of lower surface brightness. This area shows indications of tidal features, such as faint streams of stellar material. These streams are colored by yellower or reddish hues, possibly indicating a larger presence of dust.

A second distinct component is located on one side of the primary object. It is physically connected, by a faint bridge of material to the central part. Its light is more reddish/orange suggesting old stars. The overall structure indicates gravitational disturbance.
