The galaxy presents as a centrally concentrated spheroid of light, characteristic of an elliptical morphology. The core exhibits a bright, relatively uniform yellow hue. The luminosity gradually diminishes moving outward from the center, forming a diffuse halo. There is no discernible spiral arm structure or dust lane obscuration visible within the image. The galaxy appears relatively smooth in texture, with a slight elongation in its overall shape. There are no apparent signs of ongoing major mergers or significant tidal disturbances, although some minor irregularities in the outer halo cannot be ruled out. The observed color suggests a population dominated by older stars, implying a low star formation rate.
