The object presents as a galaxy undergoing a significant interaction, potentially a merger. The system is dominated by two distinct luminous components. The northern component exhibits a smoother, more diffuse morphology, appearing elliptical in shape and demonstrating a yellow-white coloration, suggestive of an older stellar population. The southern component is more compact, exhibiting a reddish hue, potentially indicative of either significant dust obscuration or a population of redder, evolved stars and active star formation. There is some visible tidal disturbance between these two, suggesting a dynamic and ongoing merger process.
