The galaxy presents an elliptical morphology, appearing relatively smooth and lacking prominent spiral arms or a distinct disk structure. Its color profile suggests a primarily older stellar population, with a yellowish-red hue dominating the galaxy's overall appearance. There is a slight elongation, with axial ratio suggesting it is not perfectly spherical. No signs of significant tidal disturbances or ongoing major mergers are observed. The absence of strong blue light indicates a lack of substantial ongoing star formation.