The galaxy presents as a spiral, exhibiting a well-defined disk structure with a discernible central bulge. The spiral arms are tightly wound. The disk appears nearly face-on to our line of sight. The bulge component appears substantial, showing a yellow-white color, suggestive of an older stellar population. The spiral arms display a bluer hue, consistent with ongoing star formation. There appear to be multiple spiral arms emanating from the central region, though precise counting is difficult. The galaxy does not display any obvious signs of a major ongoing merger, though there appears to be some distortion to the shape of the disk. There are no apparent indications of a strong bar structure in the central region of the disk. 
