The galaxy presents as a centrally concentrated, elliptical structure. There is a smooth, featureless appearance to the light distribution. The central region exhibits a bright, somewhat diffuse core, with the intensity gradually decreasing towards the outer edges. The overall color is a blend of yellow and red, suggesting an older stellar population. A subtle disk-like structure may be present, but this is not well-defined. There is no evidence of spiral arms or significant dust lanes. No significant morphological disturbances or signs of recent mergers are apparent.
