The galaxy appears as a centrally concentrated, roughly elliptical object. It exhibits a smooth, featureless morphology with a dominant spheroidal component. The galaxy presents a yellowish-orange hue, indicative of an older stellar population and a lower rate of ongoing star formation. There is a slight elongation, but overall the galaxy appears close to round. No prominent spiral arms or significant dust lanes are discernible. There are no signs of any current major merger events or tidal disturbances and appears to be isolated.
