The galaxy appears to be a relatively smooth, elliptical galaxy. It is concentrated at the center, appearing nearly round in shape. There is a slightly fainter extension of light, giving a very diffuse disk-like appearance in a very small area. No distinct spiral arms or bar structures are visible. The galaxy has a luminosity consistent with a galaxy with a stellar mass in the range of 10^10 solar masses. The color distribution suggests a population dominated by older stars, with an estimated star formation rate much lower than 1 solar mass per year. There are no obvious signs of ongoing major merger activity, although some minor disturbances cannot be ruled out at this resolution.
