The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population. The overall color gradient transitions gradually outwards from the core towards a slightly redder tone, implying a possible radial variation in stellar age or metallicity. There is a subtle hint of a disk-like structure, but the dominant characteristic is spheroidal. No strong signs of recent major merging events are apparent. Overall it appears to be a massive galaxy with very little star formation.