The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue that gradually fades into a more diffuse, red-shifted outer halo. The overall shape is slightly elongated. There is no readily discernible spiral structure or distinct features such as dust lanes, tidal tails, or prominent star-forming regions. No significant signs of recent or ongoing major merger activity are apparent. Faint disturbances in the outer halo may be present, but further, deeper observations would be required to confirm this.
