The galaxy displays a distinct spiral morphology. Two prominent spiral arms emanate from the central bulge, exhibiting a moderately wound structure. The arms appear relatively symmetrical, tracing a substantial portion of the galactic disk. The central bulge is moderately sized, and the galaxy may have a weak bar structure crossing the central bulge. No signs of major interaction or tidal disturbance are visible in the image, suggesting it is a relatively isolated system. The color gradient indicates older stellar populations in the central bulge. The light is fainter in the disk and spiral arms.
