This galaxy appears to be a spiral galaxy, presented in a face-on orientation relative to our line of sight. Distinct spiral arms are visible, though they are tightly wound around the galactic center. The central bulge is prominent and exhibits a moderate size in relation to the overall galactic disk. A bar structure is possibly present, but not very prominent, which may be related to the spiral arms. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, based on its smooth, symmetrical morphology, however minor disturbances can not be ruled out. The color profile suggests the presence of both older stellar populations, particularly within the bulge, and ongoing star formation in the arms, indicated by bluer regions within the spiral arms. Overall, the galaxy presents a classic spiral structure with a well-defined bulge and arms.