The galaxy presents as a largely featureless elliptical system. It exhibits a centrally concentrated, bright core region that transitions smoothly to a diffuse outer halo. The color profile suggests a population of older stars, with a noticeable shift towards redder hues in the central region and a diminishing of bluer components. There is a slight elongation present in the galaxy's shape. Overall, the galaxy appears to be a relatively undisturbed system, showing no strong indications of recent major merger events. Minor disturbances or the presence of a faint disk component cannot be entirely ruled out.
