The galaxy presents a morphology suggestive of an ongoing merger or close interaction between two distinct galactic structures. Both primary components exhibit an elliptical appearance, although disturbed, with elongated halos suggesting tidal interactions. There is an apparent strong red color in the core, and the outer regions appear somewhat more diffuse and feature a green hue. The overall structure seems relatively compact, with an estimated diameter of approximately 6.5 kpc, but the irregular shapes and disrupted appearance hint at dynamical processes influencing their shape and morphology. The general smoothness of each structure indicates a potentially older stellar population dominating the light output, with some ongoing star formation. The relatively smooth morphology is interrupted by signs of disturbances, which would imply that the merger is ongoing. There does not seem to be a strong dust presence.
