The galaxy presents as a centrally concentrated, elliptical morphology with a smooth appearance. The core exhibits a bright, yellowish-white glow, indicative of a high concentration of older stellar populations. Moving outward from the core, the light intensity gradually decreases, forming a diffuse halo. The galaxy shows minimal evidence of spiral arm structures or dust lanes, suggesting a lack of significant ongoing star formation. There are no visible signs of tidal disturbances or mergers, indicating it is a relatively isolated and evolved system. The shape is somewhere between round and elliptical.
