This galaxy presents as a system with disturbed morphology, likely undergoing a significant interaction. The object appears to be composed of two distinct nuclei, each exhibiting a central concentration of light. These two nuclei are embedded within a diffuse halo of lower surface brightness material.

The overall color gradient suggests a mix of stellar populations. The core regions exhibit a yellowish-white hue, which could indicate the presence of older, more evolved stars. Faint bluish tints are observed, suggestive of ongoing or recent star formation. The system displays tidal features or extended structures, which imply gravitational interaction and material exchange between the components. These features appear faint. The object exhibits signs of potential merging activity, with noticeable tidal features and potential distortions in the overall structure.
