The galaxy exhibits a clear spiral structure. Multiple arms emanate from a bright, yellowish central bulge. The spiral arms appear tightly wound, with a relatively high arm count visible. There appears to be a weak bar structure. The arms display a bluer color, suggestive of ongoing star formation. The galaxy possesses a moderate inclination, presenting a partially face-on view. The disk appears prominent relative to the bulge. There is no evidence of any significant ongoing merger activity.