The galaxy presents as a spiral type. A notable bulge is present, appearing moderately sized in relation to the disk. Distinct spiral arms are visible, exhibiting a somewhat flocculent structure. Patches of bluer light, suggestive of active star formation regions, are scattered throughout the arms. A subtle bar structure may be present, though not prominently defined. The overall morphology indicates a system that may be undergoing a minor interaction or experiencing internal disturbances, evidenced by the asymmetric arrangement of its spiral arms and the uneven distribution of star-forming regions.
