The galaxy presents as a spiral type, with two prominent, loosely wound arms emanating from a central bulge. The arms exhibit a patchy, somewhat flocculent structure, suggesting regions of active star formation. The bulge appears relatively small and diffuse, with a color indicative of an older stellar population. There's a noticeable asymmetry in the arm structure, hinting at a possible minor gravitational interaction. The overall color profile suggests a mix of stellar populations, with bluer regions in the arms indicating younger, hotter stars.
