The galaxy exhibits a prominent disk structure, not viewed edge-on, presenting a significant portion of its face. Spiral arms are readily apparent, with a morphology suggesting a grand design, and demonstrating primarily two spiral arms. These arms appear loosely wound, and the central bulge is of moderate size.

The galaxy displays a color gradient; the central region shows a yellowish-red hue, indicative of an older stellar population, while the outer spiral arms exhibit bluer tinges, suggesting ongoing star formation. No sign of a strong bar structure is evident. There is a distinct lack of any major merging or tidal disturbances in the galaxy's morphology. The galaxy appears to be in a relatively isolated state.
