The galaxy appears to be a relatively smooth, elliptical galaxy. Its core exhibits a concentrated, yellowish hue indicative of an older stellar population. There is some suggestion of tidal disturbance and potential ongoing or recent merger activity, given the asymmetry, and possible faint features extending from the central body. The galaxy appears to be roughly intermediate in roundness, and although there may be small features they appear faint in the image. There is very little evidence of blue light or active star formation visible within the galaxy itself. The mass is likely very large for the galaxy.
