The galaxy presents a largely smooth morphology with a dominant central bulge. Some features possibly indicative of a disk are suggested by the slight elongation along the vertical axis. The overall shape appears to be somewhat rounded. Evidence of a possible ongoing or past merging event is suggested by the disturbed morphology that is seen around the galaxy. A tidal tail-like feature emanates from the galaxy, further supporting the merger hypothesis. The galaxy exhibits a color gradient, with the central bulge appearing more yellow, suggesting an older stellar population, while the outer regions appear slightly bluer.
