The galaxy presents as a face-on spiral with a prominent central bulge. The spiral arms are well-defined, exhibiting a moderate winding pattern. Two dominant spiral arms are discernible. The central bulge appears significant in size, with a smooth, concentrated distribution of light. Some asymmetry or minor disturbances can be seen in the outer regions of the disk, potentially indicating a past or ongoing interaction. Overall, the galaxy displays a notable spiral structure with a relatively bright and compact core.
