The galaxy exhibits a spiral structure with tightly wound arms. The central bulge appears relatively small in comparison to the overall size of the galaxy. The arms appear somewhat flocculent, lacking clearly defined edges. There is some visible patchiness within the spiral arms, suggesting regions of active star formation. The galaxy appears to be relatively isolated, showing no strong signs of a major merger or significant tidal disturbances. The overall color is bluish in the arms, suggesting a younger stellar population, while the bulge exhibits a yellower hue, potentially indicating an older stellar population.
