The galaxy presents as a spiral type, displaying distinct spiral arm structures. The arms appear relatively well-defined. The winding of the spiral arms could be considered medium. The overall color suggests a moderate level of star formation activity, with a mixture of older stellar populations. The central bulge is visible but appears to be of moderate size compared to the overall disk. There is some asymmetry in the galaxy's morphology, possibly indicating a minor gravitational interaction or internal disturbances. There is no distinct presence of a central bar.
