The galaxy presents as an elliptical morphology, with a high degree of smoothness and a relatively round shape. The central region exhibits a high surface brightness, appearing a yellow-orange hue, potentially indicating an older stellar population. There are no discernible spiral arms or a prominent disk structure. The overall color suggests a lack of significant ongoing star formation. There are no signs of any recent or ongoing major mergers or tidal disturbances. A slight asymmetry in the outer regions is present. The galaxy shows a radial color gradient, becoming bluer at greater distances from the center.
