This galaxy appears to be relatively compact, with an elliptical morphology. A bright, concentrated central bulge dominates the structure. The outer regions show a bluer hue suggesting the presence of younger stellar populations compared to the central bulge. There appears to be a faint indication of a possible tidal tail or plume extending to the left side of the image, implying a potential past interaction with another galaxy. The overall light distribution is smooth, but there is a hint of some irregularities at the edge of the main body, possibly dust lanes or disrupted spiral arms.
