The galaxy appears to be an elliptical or lenticular galaxy. The light distribution is relatively smooth and centrally concentrated, with a yellowish-orange hue indicative of an older stellar population. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat elongated but not highly flattened. There is no obvious spiral arm structure or distinct dust lanes visible, suggesting a lack of ongoing significant star formation. Faint blueish regions can be observed, which may indicate lower levels of recent star formation. There appears to be no other distinct object indicative of a major merger, but there is a slight asymmetry which indicates a minor disturbance.
