The galaxy presents as a single, concentrated object. It appears largely featureless, with a smooth, elliptical morphology. The central region exhibits a high degree of luminosity, transitioning into a more diffuse halo. The light distribution suggests a spheroid-dominated system. There is no visual evidence of spiral arms, bars, or significant tidal disturbances. The overall color is relatively uniform, suggesting a population of older stars. There may be a slight color gradient with the central core region appearing more yellow and the outer region more blue. The absence of clear structural details indicates the galaxy is relatively relaxed and evolved. The galaxy appears isolated, without any signs of nearby companions or mergers.
