The galaxy presents as a spiral galaxy, observed at an inclined angle relative to the observer. It exhibits a clear disk structure with a distinct central bulge. While the spiral arms appear tightly wound, they are still well-defined and discernible. The luminosity distribution suggests a relatively high degree of central concentration. There is no obvious indication of any major ongoing merger or significant disturbance to the overall structure of the galaxy. The galaxy's color is a result of the combined light from its stellar populations, ionized gas, and dust.
