The galaxy presents as a relatively smooth, centrally concentrated structure with a predominantly elliptical morphology. There is minimal discernible evidence of spiral arms or a significant disk component. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in its outer regions to a more reddish color toward the core, which may be indicative of older stellar populations congregating toward the galactic center. There are some possible very minor disturbances surrounding the galaxy but I would want to investigate this further to be certain. The general roundness suggests a lack of ongoing major mergers or significant tidal interactions. The galaxy does not display strong evidence of prominent star formation regions.