The galaxy presents as a luminous, elliptical structure. There is a smooth, diffuse glow with a concentration of light towards the center that likely indicates a spheroidal component. The galaxy appears to have a relatively high degree of central concentration. The color profile leans towards the redder end of the spectrum, implying an older stellar population with minimal ongoing star formation. Visual inspection suggests the galaxy is relatively undisturbed, showing little sign of tidal features or major morphological disruptions, though there appears to be a very subtle hint of a tidal tail to the bottom left of the galaxy. There is a suggestion of multiple nuclei, or perhaps a slight distortion of the central brightness profile. The overall morphology can be characterized as relatively smooth, with a high degree of symmetry.
