The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits the highest surface brightness, decreasing steadily towards the outer regions. The visible light suggests a dominant population of older stars, evidenced by the redder color index in the outer regions, with a gradual shift towards bluer wavelengths in the core, potentially indicating some younger stars within. The galaxy's overall shape is not perfectly circular; it exhibits a moderate ellipticity, appearing somewhat flattened along one axis. No significant tidal features or signs of recent mergers are apparent, suggesting a relatively undisturbed evolutionary history. There is a suggestion of a very faint disk-like structure that appears to be oriented almost edge-on.