The galaxy presents as a relatively smooth and centrally concentrated structure. The core region exhibits a brighter, more intense luminosity, gradually decreasing in intensity towards the outer edges. There is a subtle change in color from the central region to the outer regions. The center shows a distinct hue, while the edges show a bluer hue. The overall form appears elliptical in projection, with no obvious spiral arm features or bar structures visible in the image. There are no major morphological disturbances or signs of an ongoing merger apparent; however, there could be minor disturbances present.
