The observed galaxy exhibits a clear spiral structure. Two prominent spiral arms emanate from a central bulge. The spiral arms appear loosely wound. The central bulge has a moderate size relative to the overall galactic disk. A bar structure is present, but it is not strongly defined. There may be some minor disturbances suggesting past interaction with another object, but appears mostly undisturbed. The color gradient suggests active star formation within the arms and a somewhat older stellar population in the bulge, which is indicated by the yellowish hue. The galaxy is not edge-on, but moderately inclined.
