The galaxy exhibits a disk-like morphology with a pronounced central bulge. The bulge appears yellow-white, indicating an older stellar population. The disk shows a bluer hue, consistent with ongoing star formation. Spiral arm structures are faintly visible, appearing tightly wound. The galaxy appears to be viewed at a slightly oblique angle, and the outer regions of the disk fade into the background, with the spiral arms indistinct in the outer edges. No signs of a major merger or strong tidal disturbances are apparent, although there appears to be a region of clumpy star formation slightly off-center within one of the spiral arms. Overall, the galaxy seems to be a relatively undisturbed spiral galaxy.
