The galaxy appears as a relatively smooth, centrally concentrated object. Its overall form is elliptical, showing a minimal disk-like structure and lacking prominent spiral arms. The light is concentrated towards the center, becoming fainter and more diffuse towards its outer edges. The core displays a slightly brighter intensity than the halo, and the colour exhibits minimal variation, possibly indicating a relatively uniform stellar population. There is no clear evidence of ongoing major mergers or significant disturbances in its morphology. The galaxy's shape is nearly circular on the plane of the sky. The light distribution and structural properties seem indicative of an early-type galaxy with low levels of recent star formation.
