This galaxy exhibits a prominent spiral structure. The central bulge appears moderately sized and yellowish in color, suggesting a population of older stars. The spiral arms are well-defined, displaying a predominantly two-arm structure that is tightly wound. The arms appear clumpy, indicating regions of active star formation, further supported by the blue hue that traces the spiral arms. There is some asymmetry in the arms, indicating past or ongoing minor gravitational interactions with satellite galaxies, though there is no major disturbance of the galaxy's form. There may be a weak bar in the central region.
