The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a round morphology with a high degree of symmetry. There are no prominent spiral arms or bar structures visible. The light distribution indicates a lack of significant star formation regions or dust lanes. The galaxy core appears to have a high concentration of older stars, based on its color. The galaxy does not show any obvious signs of recent major merger events or significant tidal disturbances. Based on these observations, this galaxy is classified as either an elliptical or lenticular galaxy. There is a blue object within very close proximity to the galaxy, likely another galaxy that may be interacting. 
