The galaxy presents a complex morphology, appearing as a central, compact, bright object. The core exhibits a bluish-white hue, suggesting the presence of relatively young, hot stars or strong emission lines. Surrounding this central region, there are indications of disturbed features. Patchy areas of what appear to be reddish material are observed along the perimeter of the object. The overall structure deviates significantly from a simple elliptical or spiral form. Based on the color distribution and irregular shape, a possible scenario is that this galaxy might be undergoing a merger event.
