The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white color, suggesting a high concentration of older stellar populations. This color becomes slightly redder towards the center, indicative of a possible aging population of stars or dust obscuration within the galactic nucleus.

Moving outwards from the core, the galaxy's color profile shifts to a slightly bluer hue in its outer regions, implying the potential presence of younger, bluer stars in the galactic disk. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a relatively regular, rounded shape, with minimal signs of major tidal disturbances or ongoing mergers. A slight asymmetry in the outer halo is present.
