The galaxy exhibits a notable disk structure with a moderate-sized bulge. Spiral arms are clearly visible, appearing somewhat tightly wound and extending from the central bulge into the outer regions of the disk. These arms display a mottled texture, suggesting active star formation regions along their lengths. The central bulge appears luminous and concentrated. There is no obvious presence of a strong bar structure, but a slight elongation in the central region could indicate a weak bar. The disk itself is viewed at an angle, but not completely edge-on, providing a good view of its overall structure. The general shape of the galaxy appears relatively undisturbed, showing no major signs of ongoing or recent major merger activity, though minor irregularities may exist. Color gradients are present, with the bulge appearing yellower/whiter than the bluer spiral arms.
