The galaxy presents a complex morphology, suggestive of an ongoing or recent interaction or merger. The overall structure appears disk-dominated, with a visible inclination. Distinct spiral arms are present, exhibiting a two-armed structure. The winding of the spiral arms is moderate. A central bulge of moderate size is present. A strong central bar feature can be distinguished within the bulge region. There are indications of significant disturbances to the galaxy's structure, implying possible interaction with another galaxy. The colour distribution shows a concentration of blue-ish light in the disk, which is indicative of recent star formation. The redder light is associated with the central regions, and the spiral arms are more prominent in the central and far right areas.
