The galaxy presents as a smooth, centrally concentrated structure. Its overall morphology appears elliptical, with a notable lack of distinct spiral arms or a prominent disk. The light distribution suggests a higher density of stars towards the galactic center, gradually decreasing outwards. Color gradients are subtle but present; the central region exhibits a slightly warmer hue, potentially indicating an older stellar population or increased dust concentration. The outer regions show hints of bluer colors, possibly suggesting the presence of younger, hotter stars, although these features are not sharply defined. There's minimal evidence of any significant tidal interactions or ongoing mergers, and the overall structure seems relatively undisturbed. The galaxy's shape is moderately elliptical, not perfectly spherical, but also not highly elongated or cigar-shaped.
