The galaxy presents as a centrally concentrated object, appearing largely smooth in texture with a dominant, spheroidal shape. There may be a slight hint of a disk, but is unlikely. There is evidence of a tidal tail, with a second less concentrated source to the left side of the galaxy. The galaxy appears to be relatively undisturbed, with no major signs of ongoing merger activity. The galaxy exhibits a color gradient, transitioning from a more reddish hue in the core to slightly bluer colors in the outer regions. The galaxy is likely to have a lower star formation rate.
