The galaxy presents as a spiral galaxy with a clearly defined disk structure. The galaxy has spiral arms that seem tightly wound, and the arms appear quite flocculent, with a noticeable clumpy morphology. The bluer color observed in the spiral arms suggests active star formation. The central bulge is prominent and appears smooth and concentrated, exhibiting a brighter, whitish-yellow hue. The disk is noticeably elongated with an estimated ratio of the semi-minor to semi-major axis of roughly 0.7. There are no obvious signs of strong tidal disturbances or major mergers in progress. The morphology suggests a galaxy with a moderate-sized bulge and ongoing star formation within its spiral arms.
