The galaxy presents a somewhat irregular morphology, exhibiting a disk-like structure with notable disturbances. The overall color profile suggests active star formation, with a blue-shifted distribution appearing throughout its visible structure. There is evidence of possible tidal interactions or minor mergers, indicated by asymmetries in the galaxy's shape. The northern region exhibits a diffuse, extended structure, potentially indicating a tidal tail or disrupted spiral arm. The southern region shows a brighter, more concentrated area that could be interpreted as a central bulge or ongoing starburst activity. Star clusters or HII regions are visible throughout the galaxy's arms. There are distinct regions of lower surface brightness, suggesting variations in stellar density and dust extinction within the galaxy.
