The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular type. There is a suggestion of a faint disk-like structure, but the overall light distribution is centrally concentrated. The core exhibits a bright, yellowish-white hue indicative of an older stellar population. The galaxy appears moderately round. There is some evidence of a minor disturbance, but the object shows no obvious signs of a major ongoing merger event. The galaxy exhibits a red shift and is moderate in size.
