The galaxy presents a disk-like morphology with an inclination that allows us to observe some spiral structure. While not sharply defined, there are hints of spiral arms extending from a central region. The spiral arms appear somewhat flocculent, exhibiting areas of enhanced star formation. The central bulge is relatively small, and appears to have a relatively flat profile. The overall color profile of the galaxy suggests ongoing star formation, with bluer regions concentrated in the outer disk and spiral arms. The galaxy appears to be relatively isolated, and the presence of the spiral arms suggests that the galaxy has not recently undergone a major merging event.
