The galaxy presents as a disrupted system, likely undergoing a significant interaction or merger. A primary, centrally located body exhibits a smooth, albeit irregular, morphology with a radial color gradient, suggesting a concentration of older stellar populations toward the center. Extending outwards is a complex, multi-component structure. A prominent arm or tail-like feature emanates from the central body, exhibiting a brighter, more intensely colored region suggestive of active star formation within this feature. The overall morphology indicates considerable tidal disturbance. The presence of extended diffuse light suggests recent or ongoing gravitational interactions are stripping material from the main galactic body. The system appears relatively massive. The galaxy presents evidence of star formation.
