The galaxy presents as a centrally concentrated, relatively smooth object. There is a notable lack of distinct spiral arm structure, suggesting a classification leaning towards an elliptical or lenticular galaxy. The light profile appears largely uniform with a slightly elongated shape; axial ratio is close to 1. The overall color is a blend of blue and white tones. It exhibits a soft blue hue, which could be indicative of recent star formation activity, though the general smoothness suggests this is minimal. There are no clear indications of major disturbances or ongoing mergers. Faint hints of a disk-like component are potentially present, though not prominently defined. The galaxy’s core is bright, with the luminosity gradually decreasing toward the outer regions.
