The galaxy presents an irregular morphology, with evidence suggesting an ongoing or recent merger event. The light distribution appears clumpy and disturbed, with a dominant central region showing signs of tidal features or disrupted spiral arms. The overall color is bluish, suggesting the presence of relatively young stellar populations and active star formation, with a notable fraction of the galaxy's light emitted at bluer wavelengths. It exhibits a moderate size, typical of a dwarf or intermediate galaxy. The degree of rotational symmetry appears low, consistent with a system undergoing gravitational interactions that are disrupting its internal structure. There is a large central bulge with significant star forming regions.
