The galaxy in the image presents as a spiral galaxy viewed at a slight angle. Distinct spiral arms are visible, emanating from a central bulge that appears relatively small compared to the overall disk size. The arms exhibit a somewhat flocculent structure, rather than being tightly wound. Within the arms, there are hints of brighter regions, possibly indicative of ongoing star formation. A small bar is suspected within the central part of the galaxy. The disk appears relatively undisturbed, with no major signs of a significant merger event, only very minor disturbances. Overall, the galaxy exhibits a bluish hue in the arms, suggestive of a population of young, hot stars.