The galaxy presents as a centrally concentrated object with a generally smooth appearance. There is some slight indication of possible disk features, but the galaxy is largely spheroidal in shape. There are no obvious signs of a recent major merger, although a minor disturbance cannot be ruled out. The central region appears to be dominated by older stellar populations, indicated by a redder color, with a slight decrease in color toward the outer edges of the galaxy, indicating more recent or ongoing star formation there.
