The galaxy presents as a concentrated spheroid with a bright, well-defined central bulge exhibiting a yellowish hue. The outer regions appear more diffuse, fading gradually into the background. These regions seem to show subtle hints of spirality. The galaxy has an elliptical shape with a major axis that is slightly longer than the minor axis. The overall color profile suggests an evolved stellar population, characteristic of galaxies that have ceased significant star formation activity or have undergone a burst of star formation in the past.
