The galaxy presents as an elliptical morphology with a smooth, featureless appearance. The light distribution is concentrated towards the center, with a gradual decrease in surface brightness towards the outer regions. Its overall color profile appears to be redder than many spiral galaxies. This redder color suggests an older stellar population. There are no discernible spiral arms or dust lanes. The shape is mildly elongated, but primarily round. There is no evidence of a significant ongoing merger event or major disturbances in its morphology. Minor asymmetry cannot be ruled out with the information available.
