The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a high degree of central concentration with a bright core that gradually fades into its outer regions. The color profile is predominantly redder, suggesting an older stellar population with reduced ongoing star formation. There is little to no visible disk structure or spiral arms. No signs of significant tidal disturbances, major mergers, or active galactic nuclei are apparent. The overall appearance is indicative of a well-formed and relatively undisturbed system.
