The galaxy presents a generally smooth, elliptical morphology. Its light profile is concentrated towards the center, displaying a bright, nearly spherical core. The color appears primarily yellow, suggesting an older stellar population dominates the galaxy's composition. There is little evidence of spiral arm structure or dust lanes in the image, indicating the galaxy is likely an early-type galaxy with relatively low current star formation. No signs of major mergers or significant tidal disturbances are apparent. A gradual decrease in luminosity is observed from the core outwards, forming a diffuse halo. 
