The galaxy presents as a late-type spiral, observed nearly edge-on from our vantage point. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge region. The bulge appears smooth, with a somewhat rounded morphology. The galactic disk is relatively thin and elongated. There is minimal evidence of significant star formation activity throughout the disk, as indicated by the lack of bright HII regions. A slight hint of bluer colouration is apparent in the outer edges of the disk. No significant tidal features or obvious signs of recent major merger activity are apparent in the visible light. Subtle indications of minor disturbances cannot be ruled out based on the observed morphology.
