The galaxy presents as a fairly smooth, centrally concentrated object. Its overall shape appears generally round. There is a discernible central bulge, appearing brighter and more concentrated than the outer regions of the galaxy. The color of the bulge is slightly more yellow than the surrounding galactic disk. The galaxy shows very little evidence of spiral arm structure or prominent dust lanes. There are no indications of active merging or significant tidal disturbances. The galaxy appears relatively undisturbed. The overall color suggests a higher concentration of older stars, with potentially lower current star formation.
