The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, exhibiting a high degree of roundness in its overall shape. There is little evidence of spiral arms or significant disk-like features. The color profile suggests a dominant older stellar population. The galaxy does not show signs of major mergers or strong tidal disturbances and possesses an apparently undisturbed structure. It exhibits a compact size with a high degree of central light concentration.
