This galaxy exhibits a clear spiral structure with prominent, well-defined arms extending from a central bulge. The bulge appears relatively moderate in size compared to the overall galactic disk, and displays a yellowish hue, suggesting an older stellar population. The spiral arms, in contrast, exhibit a more bluish tint, indicative of ongoing star formation regions. These regions appear somewhat patchy, but prominent, and show clear evidence of active starbirth. The galaxy doesn't appear to be strongly edge-on, allowing for a good view of its spiral structure. There are no obvious signs of a strong bar structure, though a mild bar cannot be entirely ruled out. There is a distinct lack of obvious signs of major mergers or significant disturbances, though a potential minor interaction can't be ruled out. The overall structure suggests a galaxy with relatively well-formed and defined features that is not especially smooth.
