The galaxy presents as a spiral type, exhibiting prominent spiral arms emanating from a central bulge. The arms appear relatively tightly wound. The central bulge has a moderate size and exhibits a yellowish hue, potentially indicating an older stellar population. The spiral arms display a bluer color, suggesting ongoing star formation. Dark dust lanes are visible within the arms, contributing to the overall structure. The galaxy does not show any obvious signs of major merger activity, although subtle irregularities could indicate minor disturbances or interactions. The arms appear to be grand design in nature but are somewhat fuzzy or flocculent. It appears there are likely 3 or 4 spiral arms, although due to the angle it is difficult to say for sure. It does not appear to be a barred spiral galaxy. The galaxy presents a smooth and diffused appearance. It is not presented as an edge-on disk.
