The galaxy presents as a disturbed system, likely undergoing a merger or recent interaction. It does not appear to be a standard elliptical or spiral morphology. The overall structure exhibits an irregular shape, characterized by diffuse light distribution across its components. There is the suggestion of a primary central mass, and a secondary feature attached by an extended arm. The galaxy exhibits a blue color profile, which indicates younger stellar populations or active star formation within the system. There are some areas of redder hue, suggesting the presence of older stellar populations. Evidence suggests the presence of significant ongoing star formation, particularly evident from the blue color and the disrupted morphology.
