The galaxy presents as a system undergoing interaction. The primary component exhibits a smooth, somewhat elliptical morphology, with a centrally concentrated luminosity profile. A secondary component is visible, appearing more disturbed and less centrally concentrated. Its color is noticeably redder. This suggests a higher prevalence of older stellar populations and potentially greater dust extinction. Tidal features appear to connect the two components, indicative of gravitational interaction. Overall, this galaxy displays characteristics consistent with a merging system, likely in an intermediate stage of interaction where distinct nuclei are still discernible. The apparent tidal distortion and color variations suggest differential star formation histories between the two interacting components.
