The galaxy in the image exhibits a prominent spiral structure. The spiral arms are tightly wound and somewhat patchy, appearing to originate from a moderately sized central bulge. The bulge component displays a yellowish-white hue, suggesting an older stellar population. The spiral arms are bluer in color than the bulge, indicating ongoing star formation. Two main arms can be clearly identified. No signs of significant tidal distortion are observed. There is a potential, subtle, bar feature running through the central bulge, but the resolution is not high enough to confirm. The galaxy appears relatively undisturbed.
