The galaxy presents a distinct spiral structure, viewed at an angle tilted somewhat from edge-on. Two prominent spiral arms emanate from a central bulge. The arms exhibit a patchy texture, indicative of active star formation regions. A bar-like structure appears to bisect the central bulge, running along the major axis of the galaxy's disk. The bulge itself is moderately sized relative to the overall disk. The winding of the spiral arms appears to be intermediate. There are no obvious signs of a major merger, but a possible minor disturbance is noticeable.
