The galaxy presents as a face-on or nearly face-on spiral. It exhibits a bright, prominent central bulge. From the core, spiral arms emanate outwards, displaying a degree of winding. The arms appear somewhat tightly wound in certain regions, and moderately wound in others. Patchy regions of bluer light are observed along the spiral arms, suggesting active star formation. Redder areas appear sporadically throughout the disk, possibly indicating the presence of older stellar populations or dust lanes. The galaxy displays an overall organized spiral structure. There is no obvious indication of a strong central bar feature, however, a faint, possibly nascent bar structure cannot be ruled out. The disk exhibits some mild disturbances, but shows no clear signs of a recent major merging event, yet, there seems to be some irregularity within the spiral structure.