The galaxy presents as a merging system, characterized by two distinct nuclei, each embedded within a broader, diffuse halo of stellar material. One of the nuclei displays a yellowish-orange hue, suggestive of an older stellar population, while the other exhibits a bluish tint, potentially indicating ongoing star formation or a younger stellar population. Faint, distorted tidal features are observed extending outward from the main bodies, providing further evidence of gravitational interaction. The overall shape is irregular and lacks a well-defined spiral or elliptical structure.
