The galaxy presents as a spiral type, possessing discernible spiral arm structures extending from a central bulge. The arms themselves exhibit a somewhat flocculent morphology. A bar structure bisects the central bulge. The bulge appears moderate in size relative to the overall galactic disk. Color gradients are observable, with a yellower hue concentrated towards the central bulge, indicative of an older stellar population. The disk shows bluer colors, perhaps due to recent or current star formation. There is no strong indication of major ongoing mergers or significant tidal disturbances. The galaxy is viewed at a near face-on orientation, with little inclination relative to the observer's line of sight. 
