The galaxy presents as a centrally concentrated, elliptical structure. It exhibits a smooth, relatively featureless morphology with a dominant spheroidal component. The galaxy's color appears to be moderately red, suggesting an older stellar population with a lower rate of ongoing star formation. There is no obvious disk or spiral arm structure visible. The galaxy appears largely undisturbed, without signs of a major merger or tidal interactions. Faint irregularities may be present in the outer isophotes, but these are difficult to discern.
