The galaxy presents as a spiral type, observed at a near face-on orientation. It exhibits a prominent central bulge, which appears yellowish-white. Fainter, somewhat tightly wound spiral arms extend outward from the central region, displaying a bluer hue, suggestive of active star formation. These arms have a flocculent structure, showing areas of both high brightness and low brightness, rather than smooth and continuous brightness. The disk of the galaxy is moderately inclined, showing a high amount of symmetry. There is no obvious bar structure across the central bulge. The galaxy appears relatively undisturbed with no major signs of recent merger activity or tidal distortions, presenting a well-defined spiral morphology.
