The galaxy exhibits a clear spiral structure, viewed at an oblique angle. Two dominant spiral arms are discernible, tightly wound around a moderate-sized central bulge. The arms display a relatively smooth texture, with subtle color variations suggesting regions of differing stellar populations or dust concentrations. The bulge appears yellowish, potentially indicating a population of older, redder stars. The disk of the galaxy shows a bluish tint, suggesting ongoing star formation within the spiral arms. There is no apparent bar structure. Overall, the morphology indicates a relatively undisturbed spiral galaxy with active star formation. No major signs of tidal disruption are visible.
