The galaxy presents as a spiral structure, oriented at an angle that is neither face-on nor edge-on, allowing for a clear view of the spiral arms. It exhibits a distinct disk component with relatively well-defined spiral arms. The central bulge appears moderately sized. The spiral arms seem predominantly to have a medium winding. Two spiral arms are clearly visible. There is no evidence of significant ongoing merger activity, though a minor disturbance cannot be ruled out. Overall, it seems that a bar is present.