This galaxy presents as a spiral galaxy with a significant disk component. The spiral arms are prominent, displaying a two-armed structure, although the exact number is difficult to ascertain. The winding of these spiral arms appears moderate, neither tightly wound nor loosely defined. Patches of blue light are visible, interspersed along the arms, suggesting the presence of ongoing star formation. 

The central bulge appears moderate in size relative to the disk, exhibiting a yellow-orange hue that could indicate an older stellar population. The disk of the galaxy displays a clear rotational structure, with a slight tilt relative to our line of sight, but is far from edge-on. There are some faint distortions and asymmetries observable, but are not significant enough to suggest a major ongoing merger event. A bar is seen, but it is somewhat weak.
