The galaxy presents a disturbed morphology, exhibiting characteristics suggestive of an ongoing or recent merger event. The overall shape is irregular, not displaying a clear spiral or elliptical structure. Several distinct luminous regions are visible, potentially representing the cores of the merging galaxies or areas of intense star formation triggered by the interaction. The central region appears diffuse and less structured. There's a hint of tidal tails extending outwards, albeit faint, which further supports the hypothesis of a gravitational interaction. Color gradients within the galaxy suggest varying stellar populations. The generally red color indicates the dominance of older stars and possibly a high dust content, contributing to the obscured star formation.
