The galaxy presents as a face-on spiral with a relatively bright central bulge. The bulge appears yellow, suggesting an older stellar population with a lower rate of star formation in this region. Distinct spiral arms are visible, displaying a predominantly blue hue, indicative of ongoing star formation within these structures. The spiral arms exhibit a moderately wound morphology, with primarily two arms readily discernible. The disk of the galaxy appears slightly disturbed, hinting at possible recent minor interactions or internal processes affecting its structure. There is some evidence of a bar feature crossing the central bulge.
