This galaxy presents as a spiral type, exhibiting well-defined spiral arm structures. The arms are moderately wound, neither tightly coiled nor loosely extended. A central bulge region is apparent, appearing of moderate size relative to the overall galactic disk. The bulge exhibits a yellowish hue, suggesting a population of older stars. The disk shows bluer regions indicating the presence of younger stars. The disk structure is not perfectly symmetric, potentially indicating minor gravitational interactions or disturbances. Overall, this galaxy is disk-dominated. There is no evidence of a strong bar structure in the central region.
