This galaxy exhibits a prominent disk structure viewed at a slight angle, but very close to face-on. The central bulge is of moderate size, appearing yellowish in color, suggesting an older stellar population. Spiral arms are visible extending from the central bulge, though their structure appears somewhat irregular, with several areas of intense star formation indicated by the bluer concentrations within the arms. There are indications of gravitational disturbances, suggesting possible interactions with other galaxies. Overall the galaxy is a medium sized spiral that appears to be in the process of merging with another galaxy.