The galaxy presents a discernible disk structure, with a notable central bulge. Spiral arm structures are visible, exhibiting a grand design morphology with arms that appear relatively tightly wound. The overall color profile suggests active star formation is present, particularly within the spiral arms, indicated by their bluer hue. A prominent bar structure appears to traverse the central region of the galaxy. The bulge exhibits a yellow-orange color, which could signify an older stellar population compared to the bluer spiral arms. Overall, the galaxy appears to be relatively undisturbed, showing no obvious signs of major merging events.
