The galaxy exhibits a clear disk-like structure, observed nearly edge-on from our vantage point. The central bulge appears prominent, with a primarily rounded morphology. The galaxy shows a bluer hue at the apparent edges of the disk, indicating potential areas of active star formation. The main body is reddish and yellow, suggesting an older stellar population. The morphology implies the galaxy is relatively undisturbed, with no significant signs of major mergers, though some minor irregularities within the disk cannot be ruled out. The galaxy appears well-defined and fairly smooth, though some details are lost to the limited resolution.
