The galaxy presents as a face-on spiral with a prominent central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer spiral arms extend outward from the central bulge, with some indication of patchy star formation regions within the arms. The spiral arms are moderately wound. No large scale disturbances or signs of major recent merger activity are obviously apparent. The galaxy disk appears more massive than the bulge. There is a suggestion of a bar-like structure.
