The galaxy presents a well-defined spiral structure. Two prominent spiral arms extend outwards from the central bulge, exhibiting a relatively tightly wound morphology. The arms appear somewhat flocculent, with interspersed regions of active star formation that are visibly blue. The central bulge is bright and exhibits a yellowish hue, suggesting an older stellar population. A bar-like structure may exist, as there is some elongation across the central region of the galaxy. The galaxy appears relatively isolated with no major signs of tidal disturbances or mergers.
