The galaxy appears to be a relatively smooth, elliptical galaxy, although it is not perfectly spherical. The light distribution suggests an older stellar population dominating the galaxy's composition. There is a concentration of light towards the center. Subtle color gradients are observed, with the central regions appearing slightly redder than the outer edges, which may indicate some differences in stellar population or dust content. There is no obvious spiral structure. There are no signs of active star formation. The galaxy exhibits no strong tidal features or signs of recent major mergers.
