The galaxy presents as a face-on spiral. It exhibits a moderately sized central bulge with a yellowish hue, suggesting an older stellar population. The spiral arms are well-defined and tightly wound, displaying a bluish color indicative of ongoing star formation. At least three distinct spiral arms can be discerned. No signs of major mergers or significant tidal disturbances are immediately apparent, though minor irregularities in the arm structure may suggest a minor interaction in the past. The galaxy appears relatively isolated, with no immediately obvious companion galaxies nearby.
