This galaxy presents as a spiral type. It exhibits a notable central bulge. The bulge appears moderately sized, with a yellow hue, indicating an older stellar population. Fainter spiral arms extend outward. These arms display a bluer tint, suggestive of ongoing star formation. A bar structure is not strongly apparent, or is subtly observed. The galaxy is observed face-on, providing a clear view of its spiral structure. The overall morphology suggests the galaxy has not undergone any major mergers recently, although minor disturbances cannot be ruled out.