This galaxy appears to be a relatively smooth, centrally concentrated system. The morphology is primarily elliptical, exhibiting a moderate degree of roundness. A bright central bulge is evident, emitting strongly in the yellow portion of the spectrum. A faint disk component is present, though subtle, surrounding the bulge. There is a suggestion of minor disturbances in the outer regions, and a faint structure in the disk, potentially indicating an ongoing or past minor interaction, but it is largely undisturbed. The color gradients suggest a mature stellar population throughout the main body of the galaxy.
