The galaxy presents as a centrally concentrated, yellowish-white elliptical or lenticular system. There is a high degree of central brightness, suggesting a significant stellar population concentrated in the core, likely an aging population. The outer regions fade relatively smoothly, and the galaxy appears moderately elongated. There is no visible spiral structure, nor any strong evidence of dust lanes or patches, suggesting a relatively quiescent system. The morphology indicates that the galaxy is relatively undisturbed, with no obvious signs of a recent major merger. The color suggests that star formation is likely minimal within the galaxy, supporting the morphological classification.