The galaxy presents as a centrally concentrated spheroid, likely an elliptical galaxy given its smooth appearance and lack of prominent disk features. It exhibits a radial color gradient, with a yellowish-white core that transitions to a redder hue in the outer regions. The galaxy is remarkably regular in shape, showing no signs of significant tidal disturbances, asymmetries, or ongoing mergers. Its integrated light suggests an evolved stellar population with relatively low star formation activity. The overall morphology points towards a galaxy that has largely exhausted its gas supply and is dominated by older stars.
