The galaxy presents as a fairly luminous, elliptical morphology with a centrally concentrated light distribution, indicating a prominent bulge. The overall color appears relatively uniform and slightly redder, suggesting an older stellar population, and/or high dust obscuration. The galaxy seems to be relatively undisturbed, displaying no obvious signs of ongoing major mergers or strong tidal interactions with other galaxies. The edges are smooth, with no significant visible star forming regions or spiral arm structures. There might be evidence of minor disturbances or slight asymmetry, but overall the galaxy looks to be mostly smooth in structure.
