The galaxy presents as a spiral type, observed face-on. A prominent central bulge exhibits a bright, yellowish hue, indicating a significant population of older stars. Spiral arms emanate from the bulge region, displaying a tightly wound morphology. Star formation is evident within these arms, visualized by bluer patches. The arms show structure, with an apparent discontinuity or some level of patchiness. There appears to be an overall symmetrical appearance, with no immediately visible signs of major galactic mergers or tidal distortions. The disk component is quite prominent, extending considerably outwards from the central bulge. A potential weak bar structure may exist through the central region.
