The galaxy appears to be elliptical in shape, exhibiting a smooth, concentrated central bulge that transitions into a fainter, more diffuse halo. The color profile suggests an older stellar population, with a yellowish hue dominating the central region. There's no evident structure such as spiral arms or a prominent disk. The galaxy appears relatively undisturbed, lacking signs of recent mergers or tidal interactions. The overall appearance is consistent with a passively evolving galaxy.
