The galaxy appears to be a relatively smooth, elliptical system. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in luminosity outward. The galaxy exhibits a yellowish-white hue in its core region, which transitions to a slightly redder color toward its periphery. There is no apparent spiral arm structure or obvious dust lane features visible in this image. The object appears largely undisturbed, showing no signs of major ongoing mergers or tidal distortions. Its overall shape is nearly circular, with a high degree of radial symmetry. The color suggests a population of older stars.
