The galaxy presents a disturbed morphology, exhibiting a primary, relatively smooth component and a distinct tidal tail. The main body appears mostly smooth, with a bright central region showing a slight elongation. The tidal tail extends outward from the main body, displaying a less distinct and more diffuse structure with hints of clumpy areas along its length. The galaxy exhibits a bluish hue, suggestive of ongoing star formation. The overall shape is irregular, indicating a potential interaction or merger event in its recent history.
