The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge that exhibits a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the galaxy transitions into a more diffuse halo of light, with a gradual decrease in brightness. The shape is generally ellipsoidal, with an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. There is no discernible spiral arm structure, dust lanes, or significant tidal disturbances visible in the image. The overall appearance suggests a relatively evolved system with limited ongoing star formation.
