The galaxy appears to be a relatively smooth, elliptical or lenticular type. The light distribution exhibits a generally elliptical shape, with the central region showing a higher concentration of luminosity. The color gradient suggests a population of older stars dominating the light output. Some subtle disturbances are seen on the edges, possibly hinting at minor tidal interactions or recent accretion events. It shows a red shift which suggests it is a fairly distant galaxy. Overall, the morphology suggests a galaxy that has undergone significant dynamical evolution, possibly through mergers or interactions, resulting in its current smooth and centrally concentrated structure. 
