The galaxy exhibits a distinct spiral structure. The arms appear somewhat patchy, with varying densities of stellar populations and dust lanes. The central bulge is prominent and appears reddish in color, suggesting an older stellar population. The disk is viewed at an oblique angle and contains both diffuse blue regions, indicative of active star formation, and darker, more obscured regions likely due to dust. There is evidence of minor disturbances or asymmetries in the spiral structure, potentially indicative of past or ongoing gravitational interactions. A weak bar structure seems to be present across the center of the galaxy.