The galaxy presents a face-on spiral morphology, exhibiting well-defined spiral arms. These arms display a tightly wound structure, emanating from a central bulge. The bulge appears relatively small and subdued, suggesting a lower concentration of older stars. The spiral arms show evidence of active star formation, indicated by patches of bluer light. The galaxy appears relatively isolated, without significant signs of tidal distortion or interaction with neighboring galaxies. The overall structure seems generally unperturbed, though the possibility of a minor past interaction cannot be completely ruled out based on visual inspection alone. The color gradient suggests a slightly more evolved stellar population, but regions of active star formation are still evident. There appears to be no strong evidence of a central bar structure.
