The galaxy presents as a spiral type, exhibiting distinct spiral arms. The arms are tightly wound and possess a flocculent structure, with evidence suggesting multiple spiral arms. The central bulge is relatively small and inconspicuous, contributing minimally to the overall luminosity profile of the galaxy. A bar structure appears to be present, although it is of moderate strength. There is a lack of evidence for any major merging events, although there appears to be a minor disturbance to the outer portions of the arms. The galaxy exhibits a blue color, potentially indicating ongoing star formation.