The galaxy presents as a largely featureless, smooth object with a concentrated central bulge. It exhibits a near-spherical morphology, appearing almost perfectly round. There is little indication of spiral arms or other distinct structures. The galaxy displays a color gradient, with a yellowish-white core transitioning to a slightly redder hue in the outer regions. This color shift may indicate a population of older stars predominating in the outer regions, while younger stars are present in the nucleus. There are no obvious signs of ongoing major mergers or significant tidal disturbances affecting the overall structure of the galaxy, although some minor disturbances can't be ruled out.
