The galaxy presents a generally smooth, elliptical morphology, displaying a concentrated central bulge that transitions into a more diffuse halo. Its overall shape appears somewhat elongated but not distinctly disk-like. Color gradients suggest an older stellar population, particularly within the central region, which exhibits a yellowish hue. There's faint suggestion of bluer stars, which is likely new star formation, in the outer regions, although the limited resolution obscures finer details. There's no clear evidence of a spiral structure, tidal tails, or signs of ongoing major mergers. The overall structure indicates a galaxy that is likely a massive and relatively evolved system. There may be some minor disturbances present.
