The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population, likely dominated by red giant stars. The light becomes fainter in the outer regions of the galaxy. There's a subtle but discernible redder component present in the galaxy's faint, outer regions. The isophotes appear largely smooth and regular, suggesting a well-mixed stellar population with no major recent merger events significantly disrupting the galaxy's overall structure. The axial ratio appears close to unity; we are observing a nearly round object. Star formation is possibly very low or near zero as suggested by the colors and overall morphology. 
