The galaxy presents a generally elliptical morphology, with a high degree of central concentration. The core exhibits a bright, yellowish-white luminosity, suggesting a significant population of older stars. Extending outward from the core, there's a diffuse, fainter halo that appears slightly flattened. The halo shows a hint of bluer color, indicating the presence of younger stars or possibly ongoing star formation, though at a low rate. There's no obvious presence of spiral arms or distinct features indicative of a disk galaxy. The galaxy appears relatively undisturbed, without significant tidal features or evidence of a recent major merger. Its shape is generally elongated, but not extremely so, falling between round and cigar-shaped.
