The galaxy exhibits a clear spiral structure. Two prominent spiral arms appear tightly wound around a central bulge. The bulge appears moderately sized, displaying a yellowish hue, potentially indicating an older stellar population. The spiral arms are characterized by a bluer color, suggesting ongoing star formation. A subtle bar-like structure is hinted within the central region. No obvious signs of major mergers or significant tidal disturbances are apparent. The disk is not viewed edge-on.
