This galaxy appears to be an elliptical galaxy with a smooth, diffuse light distribution. The central region exhibits a slightly brighter, more concentrated luminosity. The overall shape is somewhat elongated, appearing closer to an oval than a perfect circle. There is no discernible spiral structure, nor are there any obvious signs of ongoing major mergers or tidal disturbances. The galaxy's color is relatively uniform, exhibiting a slightly bluer hue in the center. Given its redshift, it is a relatively nearby galaxy. The light from the galaxy gives off a mass signature suggesting a low star formation rate. The lack of distinct features and the smooth light profile suggest a system dominated by an older stellar population.
