The galaxy presents as a spiral morphology, viewed face-on. High concentration of older stars is noted in the central bulge of the galaxy with yellowish hue. From this central region emanate spiral arms, exhibiting a flocculent structure. The spiral arms suggest a grand design with multiple arm segments emanating from the core. These arms are tightly wound near the nucleus, becoming less defined and more diffuse further from the central bulge. Star formation appears present within the spiral arms, characterized by subtle blue regions indicating the presence of younger stars and ionized gas. There is no visible active galactic nucleus, and the overall morphology suggests a relatively unperturbed system, though some regions of asymmetry or minor disturbances cannot be ruled out based on available resolution. There is no evidence of a strong central bar, which could suggest the galaxy is unbarred or possesses a weak bar structure. The relative brightness gradient from the central bulge outwards suggests a small bulge component to the system.
