The galaxy presents as a spiral structure, exhibiting a disk-like morphology. Two prominent spiral arms emanate from the central bulge, displaying a moderate winding. The bulge appears to be of moderate size, contributing significantly to the overall light profile. The galaxy is seen face-on, allowing a clear view of its spiral structure. A bar appears to be present, spanning across the central region of the galaxy, though it is not exceptionally strong. The disk is relatively smooth, with only minor disturbances evident, suggesting no recent major merger events. Star formation activity is indicated by the bluer hues observed in the spiral arms. The central bulge presents a more yellow/white color indicative of older stellar populations.
