This galaxy appears to be a relatively smooth, elliptical-type galaxy. It presents a centrally concentrated morphology with a high degree of radial symmetry. There is little evidence of spiral arm structure or significant dust lanes. The light distribution suggests a dominant spheroidal component. The galaxy appears nearly circular, indicating that it may be viewed close to face-on, but could still be an elliptical galaxy. There may be some minor disturbances present, but it is difficult to say for certain with the data given. The galaxy exhibits a red color, which is consistent with an older stellar population and lower star formation rate.
