The galaxy exhibits a spiral morphology with a central bulge that appears relatively smooth and concentrated. The spiral arms are discernible, although they lack sharply defined edges, suggesting a more flocculent structure. Star formation is evident, particularly within the arms, as indicated by the presence of regions with a bluer hue. The galaxy displays moderate signs of disturbance, potentially resulting from gravitational interactions. The size of the galaxy suggests that it is a relatively massive system. Overall, the galaxy appears to be a spiral galaxy with ongoing star formation and some indications of minor interactions or disturbances.
