The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. The central bulge exhibits a strong concentration of light, appearing a yellow-orange hue suggesting an older stellar population. There is some elongation visible, but the galaxy is generally rounded in shape. The galaxy appears to be undergoing some sort of gravitational interaction or merging process. This is evidenced by the diffuse, asymmetrical halo surrounding the main body and hints of disturbed structure. This is a massive galaxy with what appears to be a low rate of star formation.
