The galaxy presents a distinct spiral structure, exhibiting well-defined arms extending from a central bulge. The spiral arms appear tightly wound with a significant amount of branching. The color suggests active star formation, with patches of blue light tracing the spiral arms, indicative of young, hot stars. The central bulge displays a yellowish hue, potentially indicating an older stellar population. A moderate degree of asymmetry or disturbance is apparent in the galaxy's structure, possibly related to gravitational interactions or an ongoing minor merger event. There is no clear bar feature visible. The bulge seems small relative to the disk, not contributing significantly to the overall light profile of the galaxy. 
