The galaxy presents as a spiral structure with a notable central bulge. The spiral arms exhibit a defined, two-armed morphology and appear tightly wound, with an inclination that presents a partially face-on view to our line of sight. A bar structure is observed bisecting the central bulge. The bulge appears to be moderate in size. The overall color profile suggests the presence of both older stellar populations, indicated by the yellowish hue of the bulge, and younger, bluer stars within the spiral arms. There is no immediately apparent evidence of major merging or significant tidal disturbances, although some minor disturbances cannot be ruled out. The morphology appears relatively smooth, without substantial clumpy star formation regions readily visible.
