This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. The core is a dominant yellowish-white, suggesting a population of older stars, and there is a faint, diffuse blue halo surrounding it. The spheroidal shape suggests a relaxed system that is likely a low-level star-forming region. There is no obvious dust lane or spiral arm structure visible. No apparent signs of recent major merger activity are observed. The galaxy appears well-defined despite the distance.
