The galaxy presents as a moderately bright, face-on spiral with a prominent central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Spiral arms are faintly visible, displaying a bluer color indicative of more recent star formation. These arms appear somewhat loosely wound, and their structure is not sharply defined. The overall disk component of the galaxy seems relatively smooth and extended. Patches of reddish emission are observed near the outskirts, possibly representing HII regions or areas of dust obscuration. The galaxy does not appear to be undergoing any major merging events, though minor disturbances or tidal features cannot be ruled out based solely on the image.
