The galaxy presents as a spiral type, with a distinct disk structure that exhibits strong spiral arm features. These arms appear tightly wound around the central bulge region. The bulge itself constitutes a moderate portion of the galaxy's overall size. There is no apparent strong bar structure bisecting the galaxy's nucleus, although a weak bar may be present. The color distribution within the galaxy suggests ongoing star formation, particularly within the spiral arms, where a bluer hue is observed. The central bulge appears yellower in color. Overall, the galaxy does not exhibit any significant morphological disturbances, however, a minor disturbance may be occuring. The galaxy is observed at an intermediate inclination.