The galaxy presents as a relatively small, edge-on disk galaxy. A clear dust lane bisects the galaxy, obscuring the central bulge and indicating significant internal dust content. There is evidence of ongoing star formation within the disk. A bright concentration of stars is present on the right side of the galaxy, as well as some concentration towards the core on the left. Overall, the galaxy appears to be relatively undisturbed, showing no signs of major recent mergers or interactions. The general morphology indicates an actively star-forming, but otherwise relatively normal disk galaxy viewed edge-on.
