The galaxy presents as a relatively face-on spiral, displaying a well-defined disk structure. There is evidence of spiral arm structure, albeit somewhat flocculent, exhibiting a greenish color. The galaxy possesses a prominent bulge region exhibiting a reddish color, suggesting an older stellar population and/or dust obscuration. The overall shape appears to be elliptical. A bar is present with a size of moderate magnitude, although it is not very bright. There is no apparent evidence of strong tidal interactions or ongoing major mergers. There is some disruption in the disk, indicating possible minor disturbances due to possible past mergers.