The galaxy exhibits a prominent spiral structure. The spiral arms appear tightly wound and relatively continuous. The central bulge is moderately sized, displaying a yellowish hue, suggesting an older stellar population. The disk component is bluish, indicative of younger, hotter stars and ongoing star formation. The galaxy shows no strong evidence of a central bar structure. There appear to be multiple spiral arms emanating from the central region. The overall structure is relatively well-defined, with no indications of major mergers or significant tidal disturbances. There are some minor disturbances.
