The galaxy presents as a spiral type, exhibiting a prominent disk structure with visible spiral arms. The arms appear grand design-like and trace almost all the way to the inner core. The disk shows a blue-ish hue, suggesting the presence of younger stellar populations and ongoing star formation. A prominent central bulge with a yellow-orange color is evident, potentially indicating an older, more evolved stellar population. The bulge occupies a moderate amount of the galaxy. There is no obvious bar structure. The arms appear to be moderately wound. Two main arms appear to be present. No major signs of disturbance via merging are present.