The galaxy presents as a face-on spiral with a prominent central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. The spiral arms are not sharply defined but appear flocculent, with regions of bluer light indicating ongoing star formation. The galaxy's overall structure appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions. The dust lanes within the spiral arms are subtle but noticeable, hinting at a complex interstellar medium. The central region is relatively bright, potentially hosting an active galactic nucleus or a dense concentration of stars.
