The galaxy presents as a spiral type, observed at a near face-on orientation. Its overall structure exhibits a distinct central bulge that appears somewhat elongated along the major axis of the galaxy. The bulge displays a concentrated luminosity, suggesting a significant stellar population density.

Spiral arms are evident, though their definition varies. The arms are traced by regions of bluer light, implying ongoing star formation within these areas. Dust lanes are faintly visible, particularly in the inner regions of the disk, obscuring some of the background starlight.

The spiral arms exhibit a relatively tight winding pattern. There appears to be primarily two prominent spiral arms. There is no evidence of a strong bar structure. Some asymmetry is present in the spiral arm structure. There is no obvious visual evidence of a major ongoing merger event. 
