The galaxy presents a distinct spiral structure. Two prominent spiral arms emanate from a central bulge region. The spiral arms appear somewhat flocculent and exhibit a medium degree of winding. The central bulge displays a moderate size relative to the overall galactic disk. A bar-like structure appears to be present, with a moderately strong signal. The galaxy's disk appears relatively undisturbed, without obvious signs of major mergers or significant tidal distortions. Star formation is observed within the spiral arms.
