The galaxy appears to be a spiral galaxy viewed at a significant angle to our line of sight, presenting as a flattened disk. The central bulge is prominent and exhibits a yellowish hue, potentially indicating an older stellar population and a lower rate of star formation within the bulge itself. Fainter spiral arms extend from the central bulge, displaying a bluer color which could be evidence of ongoing star formation. Dust lanes are subtly visible within the disk, obscuring some of the starlight. The overall morphology suggests the galaxy is relatively undisturbed, with no major signs of interaction or merging activity. It displays a regular structure, suggesting a galaxy that has evolved primarily in isolation.
