The galaxy presents as a spiral type, exhibiting a prominent central bulge that appears elongated. A well-defined bar structure traverses the bulge. Two primary spiral arms emanate from the ends of the bar, demonstrating a tightly wound morphology. The arms display a patchy structure indicative of ongoing star formation. The galaxy shows some signs of gravitational disturbance, with irregularities in the arm structure. There appears to be some merging going on with this galaxy. The overall color suggests a relatively mature stellar population, though pockets of bluer light point to more recent star birth.