The galaxy presents a disk-like morphology with a discernible, albeit not sharply defined, spiral structure. The spiral arms exhibit a flocculent appearance, characterized by patchy, discontinuous segments of enhanced luminosity. These segments likely correspond to regions of active star formation. The central bulge is moderately prominent, displaying a smooth, elliptical shape with a yellowish hue, indicative of an older stellar population. Dust lanes are subtly visible within the disk, particularly along the inner edges of the spiral arms, obscuring the light from background stars and gas. Overall, the galaxy appears relatively undisturbed, lacking strong signs of recent major mergers or tidal interactions. The color gradient suggests ongoing star formation within the spiral arms.
