The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms are well-defined, with a multi-armed morphology. Some areas of these spiral arms appear flocculent, with regions of increased luminosity likely indicating areas of active star formation. Other portions seem more sparse. The arms appear more tightly wound in some regions. The central bulge is small relative to the overall disk size and exhibits a moderate concentration of light, appearing not very pronounced. No evidence of a significant bar structure is visible. The disk appears relatively undisturbed, with some possibility of minor irregularities that could indicate gravitational interactions or minor mergers. A non-negligible fraction of the arms shows high star forming properties. The color suggests ongoing star formation in the disk.