The galaxy presents a spiral morphology, displaying prominent, well-defined arms. These spiral arms exhibit a relatively tightly wound structure. Two major arms appear dominant, tracing a clear path from the central region outward. The arms are somewhat patchy, possibly indicating areas of active star formation interspersed with regions of lower stellar density. 

A central bulge is observed, appearing as a concentrated region of light. The bulge is of moderate size relative to the overall galaxy. A bar-like structure is observed intersecting the bulge, though the bar appears rather weak and ill-defined.

The overall color of the galaxy suggests a mix of stellar populations. The bulge exhibits a yellowish-white hue, possibly indicating an older stellar population. The spiral arms appear bluer, indicative of the presence of younger, hotter stars within star-forming regions.
