The galaxy appears to be a single, relatively smooth object, with a high degree of central concentration. The morphology is predominantly elliptical. There is a distinct lack of spiral arm structure or significant features indicative of a disk. The light profile is relatively smooth, with a color gradient suggesting a transition from a yellower core to slightly bluer outer regions, possibly indicating the presence of a slightly younger stellar population in the outskirts compared to the center. The galaxy is compact, with a fairly well-defined boundary. There is no obvious evidence of ongoing major merging activity.
