The galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. There is evidence of spiral arm structure present within the galaxy. Predominantly two spiral arms exist, with a medium winding. The galaxy exhibits a bar feature. The bulge size is small to moderate, with no clear dominance. The overall light distribution suggests that the galaxy is experiencing a moderate amount of star formation. Based on its morphology, the galaxy is not strongly interacting with any other galaxies, but there is the presence of minor to major disturbances, with potentially minor merging.
