The galaxy presents a disk-like structure observed nearly edge-on from our vantage point. The primary color is yellow, indicative of a stellar population dominated by older stars, or potentially significant dust obscuration. A distinct central bulge is not readily apparent, however there appear to be two areas of high concentration. There is some clumpy structure. This galaxy is experiencing relatively low levels of star formation. There is potential for a minor disturbance, perhaps a merger. There is a slightly disturbed morphology. The galaxy is of substantial mass and luminosity.
