The galaxy exhibits a complex morphology, appearing as a possible ongoing merger event or a galaxy with significant tidal disturbances. The primary body of the galaxy shows a diffuse, elongated structure with a noticeable central concentration of light. There is a suggestion of a distorted spiral arm or tidal tail extending from the central region. Color variations within the galaxy indicate differing stellar populations, with bluer regions possibly signifying areas of active star formation. There is also an attached tidal feature towards the left. No clear dust lanes are visible. The galaxy is irregular in shape, lacking a well-defined disk or elliptical structure.