The galaxy appears as a relatively smooth, elliptical structure. Its color gradient transitions from a yellowish-white center to a more diffuse, blue-tinged outer region. The central bulge is dominant, with a high concentration of light, suggesting an older stellar population. The galaxy is elongated, showing an ellipsoidal shape. There is a subtle indication of a disk, but no distinct spiral arms are discernible. There is no evidence of a major ongoing merger, although there is a hint of minor disturbances in the outer regions. Overall, the galaxy appears to be a mature system, exhibiting characteristics of a relatively quiescent stage of evolution.
