The galaxy exhibits a prominent spiral structure. The spiral arms are tightly wound and extend from a central bulge. The bulge appears relatively small. The galaxy's disk is oriented close to face-on. A bar structure is suspected, but not clearly distinguished. Star formation is apparent within the spiral arms, indicated by localized blue regions. There are some signs of minor disturbances along one of the arms, but no major merger is visible. The core of the galaxy is an intense yellow color, indicating there may be older stars or a supermassive black hole at the center. 
