This galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. There is a noticeable color gradient, with the central region appearing more yellow/orange, suggesting an older stellar population and potentially higher dust concentration. The outer regions of the disk exhibit a slightly bluer hue, indicating the presence of younger, hotter stars, but at a much smaller concentration than the interior of the galaxy. There's no clear evidence of spiral arms or a distinct bulge. The overall morphology suggests a galaxy with a low star formation rate that has been ongoing, but is not especially high for a galaxy of this magnitude. There are no prominent tidal features or significant asymmetries visible in the image, indicating that no major merger events are ongoing. However, there is a slight asymmetry in the morphology of the outer disk, which is more prominent on one side of the galactic plane, possibly indicating a minor disturbance.
