The galaxy appears to be a spiral galaxy, presenting a face-on orientation. The spiral arms are tightly wound and numerous, exhibiting a flocculent structure. A notable, albeit not dominant, bulge is observed, displaying a somewhat diffuse brightness profile. There is evidence of a bar structure extending through the galactic center, though it is not particularly pronounced. Overall, the galaxy shows no immediate signs of major mergers or significant disturbances. The color indices suggest a moderate level of star formation, with bluer regions tracing the spiral arms.
