The galaxy exhibits a spiral structure, although the arms appear somewhat diffuse. They extend outwards from a central bulge. The bulge is moderately sized and exhibits a yellow-white hue, indicative of an older stellar population. The spiral arms show a bluer tint, implying ongoing star formation. The galaxy doesn't appear to be a pure spiral, rather it has a more flocculent appearance. A bar structure may be present, although if it is, it is weak. The galaxy does seem to be interacting with another system, as it is not completely settled. The disk is viewed close to face-on. There is potentially some disturbances to the system, implying that it may be merging with another galaxy.
