The galaxy presents as a face-on spiral, exhibiting well-defined spiral arms. There is a prominent central bulge. The spiral arms appear quite flocculent, with numerous HII regions visible as brighter knots of star formation. The color of the bulge appears generally yellowish, suggesting a population of older stars, while the spiral arms display bluer hues, indicative of younger stellar populations. The disk appears moderately thick. No obvious signs of a bar structure are visible at this resolution. No major signs of ongoing merger activity are seen.
