The galaxy presents as a diffuse, yellowish-orange elliptical type. It is characterized by a smooth, centrally concentrated light profile, lacking any discernible spiral arms or prominent disk-like features. Its form appears more elongated than perfectly spherical. The light distribution suggests the absence of significant dust lanes or patchy star formation regions. There are no other obvious signs of recent mergers or tidal disturbances. Based on its color and morphology, this galaxy likely consists predominantly of older stellar populations with minimal ongoing star formation.
