The galaxy presents as a slightly elongated, elliptical structure with a smooth and centrally concentrated luminosity profile. There is a bright, yellowish central region, which likely indicates an older stellar population or a concentration of dust. Surrounding the central region is a fainter, more diffuse blueish halo. This halo suggests the presence of a younger stellar population. The overall morphology of the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There may be minor indications of possible disturbances in the outer regions. Overall the galaxy appears massive.
