The galaxy presents as a face-on spiral with a discernible disk structure. Prominent spiral arms extend outward from a central bulge. The arms exhibit a moderate winding pattern, neither tightly wound nor exceptionally loose. The disk color is predominantly bluish, indicative of ongoing star formation. The central bulge appears yellowish, possibly suggesting an older stellar population. The spiral arms appear to branch into two distinct arms and have low levels of dust obscuration visible. There is no sign of interaction with any neighboring galaxies.
