The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is somewhat rounded but not perfectly spherical, appearing slightly elongated. A central bulge is clearly visible, exhibiting a high concentration of light. The color gradient transitions smoothly from a yellow-white core outwards to a redder, fainter halo. There is no apparent spiral arm structure or distinct dust lanes. Based on its morphology, it likely has a low ongoing star formation rate. There are no indications of major mergers or significant tidal disturbances affecting its structure.
