The galaxy presents as a single, relatively concentrated object. Its morphology suggests a spheroid shape, appearing somewhat rounded, although it may possess a slightly elliptical form. The galaxy's light profile indicates a smooth distribution of stars, with a high degree of central concentration. While not perfectly spherical, there is no obvious disk structure.

Color gradients are subtle. The core appears yellowish-white, while the outer regions seem subtly bluer, suggesting the possibility of some ongoing star formation. No prominent tidal tails or obvious signs of a major ongoing merger are immediately apparent. However, subtle irregularities hint at minor disturbances. The integrated light indicates a relatively luminous system, indicative of a high stellar mass.
