The galaxy presents as a face-on spiral, exhibiting a prominent central bulge that appears yellowish, suggesting an older stellar population. The spiral arms are tightly wound, emanating from the central region and displaying a mottled texture, possibly indicating regions of active star formation. These arms show a bluer hue compared to the bulge, consistent with younger, hotter stars. The disk component dominates the overall structure, with the bulge appearing relatively small in comparison. No significant bar structure is readily apparent within the central region. The overall morphology appears relatively undisturbed, showing no indications of a major ongoing merger, although minor irregularities may be present.
