The galaxy presents as a spiral type, exhibiting prominent spiral arms. The majority of the light from the galaxy is concentrated in the disk. The arms appear symmetrical. There is a moderate central bulge component that contributes to the overall luminosity. Two clear spiral arms are observed. The arms are moderately wound. There is no apparent major merging event, though the arm structure is somewhat disturbed, so potentially a minor interaction could be ongoing. The galaxy disk does not appear edge-on. The galaxy has a bar component.