The galaxy presents as a singular, relatively smooth object. The shape appears elliptical, with a high degree of roundness. The central region exhibits a bright, concentrated luminosity that gradually diffuses towards the outer edges. There is no obvious spiral structure, bar, or distinct features. A faint, asymmetrical extension or possible tidal tail could be present. The color gradient suggests a stellar population of intermediate age, with a moderate rate of star formation. There is no presence of any major disturbances or indications of an ongoing merger event.
