The galaxy appears to be a relatively face-on spiral, possibly with a weak bar structure. It presents a smooth, somewhat featureless disk, dominated by an older stellar population with little active star formation visible in the image. There appears to be a slight reddening towards the center. The galaxy exhibits a round morphology, with no major disturbances or mergers evident. There is some minor disturbance. Its color index suggests it contains both older stars and perhaps some ongoing, albeit subdued, star formation. It has a medium mass.
