The galaxy appears to be a relatively face-on spiral, exhibiting a bright, concentrated central bulge. Faint spiral arms are visible, extending outwards from the bulge. The galaxy appears relatively smooth. There is a slight asymmetry in the distribution of light within the outer regions, but the general shape is consistent with a spiral morphology. No significant tidal features or signs of ongoing major mergers are apparent, although minor disturbances cannot be ruled out. The central bulge appears yellow, possibly indicating an older stellar population and dust extinction, while the faint spiral arms exhibit a bluer hue suggestive of ongoing star formation.
