The galaxy presents as a moderately luminous, elliptical morphology with a smooth, featureless appearance. The core exhibits a concentrated, yellowish-white hue, suggesting an older stellar population. The outer regions display a gradual decrease in surface brightness, with a subtle reddening effect. No spiral arm structures or distinct dust lanes are discernible. There is no evidence of any significant tidal disturbances or merging activity. The axial ratio suggests a moderate degree of ellipticity, deviating somewhat from a perfectly spherical shape. The galaxy appears relatively isolated, lacking nearby companion galaxies that would indicate potential interactions.