The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The light appears to fade gradually outwards from the core without distinct spiral arms or prominent features. The overall shape is elliptical, trending towards a rounded appearance rather than a highly elongated form. There is no strong evidence of tidal disturbances, major mergers, or significant star formation regions visible in the available image. The smooth and symmetrical light distribution suggests a galaxy that has undergone significant dynamical relaxation. 
