The galaxy presents as a face-on spiral with a noticeable bulge. The spiral arms are well-defined, tightly wound, and exhibit a high degree of symmetry. The bulge appears moderately sized relative to the disk, suggesting an intermediate classification. There's no visual evidence of a strong bar structure. The disk shows some patchiness, possibly indicating active star formation regions along the spiral arms. No signs of major mergers or significant tidal disturbances are apparent. The galaxy shows a prominent core, and the color appears to be consistent between the core and the arms. 
