The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be largely elliptical, exhibiting a high degree of roundness with a slight deviation towards an intermediate shape. There is no prominent disk structure, and no signs of significant ongoing merger activity or major disturbances are observed. Minor disturbances are potentially present but not distinct. The color profile suggests a moderate population of older stars with a subtle blue component, suggesting low levels of recent star formation. The stellar mass is estimated to be substantial.
