The galaxy presents a discernible spiral structure, exhibiting two prominent arms extending from the central bulge. These arms display a moderate winding, neither tightly coiled nor loosely dispersed. The central bulge appears moderate in size, contributing significantly to the overall luminosity of the galaxy. There is no evidence of a significant bar structure bisecting the bulge. The galaxy exhibits a disk-like morphology viewed at a slight angle. No major mergers are apparent, although there seems to be some minor disturbance in the disc. A smooth component can be seen although the disk-like feature dominates the appearance. 
