The galaxy appears to be a relatively smooth, centrally concentrated object. Its light profile suggests a dominant spheroid component, potentially an elliptical galaxy or a lenticular galaxy seen face-on. It exhibits a slight elongation, deviating from a perfectly circular shape. There is a subtle color gradient visible, with a yellowish-white core region that gradually transitions to a bluish-white outer region. The outer disk, if present, is faint and lacks prominent spiral arm structures or distinct features. No signs of major mergers or significant tidal disturbances are visible. There might be minor irregularities in the outer regions, however, these could simply be areas with different star formations.
