The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a centrally concentrated light distribution with a high degree of circular symmetry. The core region displays a bright, yellowish hue, suggesting an older stellar population. The galaxy appears to be fairly massive with a star forming rate that is relatively low. There may be minor disturbances present but these are not easily observable. The possibility of an ongoing or recent merger event cannot be ruled out, despite the generally smooth appearance. The outer regions fade gradually into the background, with no sharply defined edges. Overall, the galaxy's morphology is consistent with an evolved system dominated by older stars and minimal ongoing star formation.
