The galaxy presents as a spiral type, with a disk that is neither fully face-on nor edge-on relative to our line of sight. The spiral arms are prominent, displaying a multi-armed structure that is somewhat flocculent in appearance. These arms exhibit distinct blue hues indicative of ongoing star formation. The disk of the galaxy shows a significant bar-like structure that spans a considerable portion of its diameter. This bar is populated with both older stellar populations, indicated by its yellower color, and regions of active star formation along its leading edges.

A central bulge is visible, although it does not dominate the overall structure of the galaxy. The bulge appears relatively compact and blends smoothly into the surrounding disk. There does not seem to be a distinct dust lane within the galaxy. No signs of recent major merger activity are apparent, although there appears to be some minor tidal disturbance on one side of the galaxy. Overall, the galaxy has an intermediate inclination angle that allows a clear view of its spiral structure, bar, and star-forming regions.
