The observed galaxy exhibits a prominent disk structure, viewed at a slight inclination. Within the disk, spiral arms are clearly discernible, displaying a relatively open morphology. These arms are traced by regions of blue light, suggesting ongoing star formation. The central bulge appears small in size compared to the overall galactic disk, and exhibits a yellowish hue, potentially indicative of an older stellar population. No apparent bar structure is detected within the central region. The galaxy shows no obvious signs of a major merger event, although a minor disturbance cannot be entirely ruled out. The galaxy's overall appearance is generally undisturbed, with a smooth profile beyond the spiral arms.
