The galaxy presents a clear spiral structure, although the arms appear somewhat tightly wound. The central bulge is prominent and exhibits a yellowish hue, potentially indicating an older stellar population. Fainter blue regions suggest the presence of ongoing star formation within the spiral arms. There is a hint of a bar-like structure crossing the central bulge. Overall, the galaxy appears to be relatively undisturbed, showing no obvious signs of a recent major merger, though there are some signs of minor disturbances.
