This galaxy exhibits a pronounced disk-like morphology, viewed at a relatively high inclination. The galaxy displays a centrally concentrated bulge component, with the majority of the light appearing to originate from an extended disk. Faint spiral arm structures appear to be present within the disk.

There are subtle color variations within the galaxy. The central bulge appears yellowish, indicative of an older stellar population. The outer disk shows slightly bluer hues suggesting more recent star formation activity. The galaxy appears relatively isolated.