The galaxy presents as a face-on spiral galaxy, exhibiting a distinct disk structure. Two prominent spiral arms emanate from the central bulge, displaying a medium winding pattern. The central bulge appears moderate in size and exhibits a yellowish hue, suggestive of an older stellar population. The spiral arms are bluer, indicating regions of active star formation. The galaxy is not edge-on, and does not show any signs of merging or major disturbance. The presence of spiral arms suggests ongoing star formation within the disk. A weak bar structure may exist within the central region.
