The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a relatively high degree of central luminosity. The overall color profile suggests a relatively evolved stellar population, with the central bulge appearing more yellow/orange than the outer regions which exhibit a bluer hue. There is a slight asymmetry on the right side of the galaxy, which has a redder color. This could potentially indicate an ongoing minor interaction or merger event, where an infalling, smaller object contributes redder light, though the galaxy appears largely undisturbed. Based on the colors and overall morphology, the galaxy's star formation rate is likely relatively low. The apparent roundness and lack of prominent spiral arms suggests this is likely an elliptical galaxy, although some disk features may be present.
