The galaxy presents as a moderately bright, centrally concentrated object. Its morphology appears to be relatively smooth, lacking distinct spiral arms or a prominent bar structure. There's a gradual decrease in luminosity from the core outwards, suggesting a significant bulge component. The overall shape is somewhat elliptical, though not perfectly spherical; it is moderately flattened. The color profile shows a yellowish-white core, transitioning to a bluer hue in the outer regions, which is suggestive of recent star formation taking place away from the bulge. The overall structure seems relatively undisturbed with no obvious signs of an ongoing major merger event. Minor irregularities in the outer regions may indicate past interactions or minor disturbances.
