The galaxy presents as a spiral galaxy with a prominent disk structure oriented at a slight inclination relative to the observer's line of sight. The central bulge region appears bright and concentrated, with a yellowish hue, suggesting an older stellar population. Two tightly wound spiral arms emanate from the central bulge. The spiral arms display a mix of bluer regions indicative of ongoing star formation and redder areas indicating the presence of more evolved stars. The disk appears relatively smooth overall with no obvious signs of major tidal disturbances or ongoing mergers. The galaxy appears to be a late type spiral with moderate dust lanes. 
