The galaxy presents as a spiral type, exhibiting a pronounced central bulge that appears approximately half the size of the full diameter of the galaxy. Two prominent spiral arms are visible, though with some degree of patchiness and flocculence. The arms appear moderately wound. There is evidence of a bar structure transecting the bulge. No strong signs of ongoing major merger activity are apparent, although some minor disturbances in the outer disk cannot be ruled out based solely on visual inspection. The galaxy displays a generally smooth appearance overall.
