The galaxy presents a complex morphology, appearing as a diffuse, irregularly shaped object. It has a dominant greenish hue, suggesting active star formation. There is a central brighter region, surrounded by fainter, more extended features. This region appears to have patchy areas. Possible signs of minor disturbances are visible as subtle asymmetries in the outer regions. The overall structure suggests an actively evolving system, possibly undergoing a minor merger or interaction that could be triggering the star formation. The galaxy's irregular shape and lack of a well-defined disk structure may suggest a transition from a more ordered system or the presence of on going disturbances.
