The galaxy presents a face-on spiral morphology. It exhibits a bright, concentrated central bulge that appears yellowish in color, suggesting an older stellar population. A disk surrounds the bulge, displaying bluer hues, potentially indicative of younger stars and ongoing star formation within the spiral arms. The spiral arms appear somewhat tightly wound and display a moderate degree of prominence and distinctness, with some areas showing clumpy regions, possibly HII regions. The galaxy appears well-formed and unperturbed, displaying no obvious signs of a recent major merger event. The light distribution suggests a relatively high degree of central concentration, but the disk contributes significantly to the galaxy's overall luminosity.
