The galaxy appears to be a spiral, viewed at a slight angle. It exhibits a prominent central bulge which appears yellow in color, suggesting an older stellar population. The disk is characterized by a patchy distribution of blue light, indicative of ongoing star formation within spiral arms. The spiral arms themselves are tightly wound around the bulge, creating a somewhat flocculent morphology. The galaxy shows no obvious signs of major tidal disturbances or interactions, though there are hints of minor asymmetry in the disk. Overall, the galaxy presents a relatively normal spiral structure with a moderate bulge and active star formation in the disk.
