The galaxy presents as a face-on spiral galaxy with a prominent, yellowish central bulge. The spiral arms are well-defined but somewhat tightly wound, displaying a bluish hue indicative of ongoing star formation. There is a possible barred structure, although it is not very distinct. The spiral arms exhibit some granularity, potentially caused by HII regions or star clusters. No apparent signs of a major merger event are observed, though there may be minor disturbances visible. Overall, the galaxy appears to be an actively star-forming system with a moderate-sized bulge.
