The galaxy appears to be elliptical in shape, with a smooth, centrally concentrated light distribution. The core region is bright and yellowish, suggesting a population of older stars. The outer regions fade gradually, displaying a redder hue. There are no obvious signs of spiral arms or prominent dust lanes. The galaxy exhibits a relatively high degree of roundness, appearing neither highly elongated nor perfectly spherical. There's no evidence of significant tidal disturbances or ongoing major merger events. The galaxy's light profile suggests that the galaxy is dominated by a bulge with relatively little or no disk structure.
