The galaxy presents as a spiral galaxy with a discernible disk structure. The spiral arms appear tightly wound, exhibiting a flocculent morphology. The galaxy possesses a prominent central bulge, which suggests a relatively early-type spiral. The disk component appears somewhat irregular, and there may be some dust lanes or patches of obscuration. The galaxy is not edge-on, and no signs of a bar are apparent. The morphology appears undisturbed, with no signs of a major merger. The galaxy has a yellowish hue, which could indicate that the galaxy is made up of older stars. 
