The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a substantial stellar population. Moving outward from the center, the light gradually diminishes, forming a diffuse halo that appears somewhat elongated. There's a possible faint disk-like structure, but it is not well defined. Some evidence of minor disturbances, such as slight asymmetries in the outer halo, is visible, but the galaxy does not show any strong signs of a major ongoing merger. The overall color is yellowish, suggesting a population of older stars with relatively low levels of ongoing star formation.
