The galaxy presents a spiral structure, although the arms are not sharply defined. Two main spiral arms appear to originate from the central region and extend outwards. The arms exhibit a winding pattern of medium tightness. The central bulge is prominent, of moderate size, and displays a yellowish hue, suggesting an older stellar population. Overall, the galaxy is relatively face-on. There is a hint of a bar-like structure bisecting the bulge, but its definition is difficult to assess. The outer disk shows a bluer tint, indicating the presence of younger stars and ongoing star formation. There is no visual indication of any major ongoing merger events.
