The object presents as a diffuse, irregular galaxy with a disturbed morphology. There is evidence of tidal features or plumes extending from the main body. The color distribution across the galaxy is not uniform, suggesting variations in stellar populations or dust content. Some regions appear bluer, indicating possible ongoing star formation, while other areas are redder, potentially indicating older stellar populations or significant dust obscuration. The overall structure lacks a well-defined nucleus or spiral arm structure, supporting the classification of an irregular morphology. There are disturbances in its form, which could indicate a minor or major merger, as there are asymmetrical shapes in its outer edges.
