The galaxy presents as a centrally concentrated, relatively smooth object. Its overall morphology appears elliptical, displaying a high degree of roundness. There is little evidence of spiral arms or a prominent disk structure. The light profile suggests a gradual decrease in surface brightness from the core outward, lacking sharp edges or distinct features. Faint color variations are observed, with a subtle bluer hue in the outer regions compared to a slightly redder central bulge, potentially indicating some ongoing, albeit moderate, star formation. No significant signs of tidal disturbances or interactions with other galaxies are apparent. Overall, it has an elliptical shape with little or no major disruptions.