This galaxy appears to be a relatively smooth, elliptical galaxy. The central region exhibits a concentrated, yellowish hue suggesting an older stellar population. The outer regions show a gradual transition to a slightly bluish color, possibly indicating the presence of a younger, though limited, stellar population or some ongoing star formation. The galaxy exhibits a slight elongation, but is mostly round. There is no obvious evidence of significant tidal distortions or ongoing merger activity. There is a possible very slight ring like structure.
