The galaxy presents as a relatively smooth, elliptical object with a high degree of central concentration. The core region exhibits a bright, nearly stellar appearance, which then diffuses outward into a more extended halo. There is a slight elongation visible along one axis, suggesting a departure from perfect circularity. Faint, diffuse features that may be indicative of a disk structure are barely visible within the galaxy. There appears to be minimal evidence of recent or ongoing merger activity; the overall structure is largely undisturbed, showing no strong tidal tails or other obvious signs of interaction. Color gradients are present, with the central region appearing whiter, suggesting an older stellar population, and the outer regions exhibiting bluer hues. The redder central regions have minimal recent star formation, and the bluer outer regions have moderate star formation.
