The galaxy presents as a somewhat smooth, elliptical-like structure. Its light profile appears centrally concentrated. There is a slight deviation from perfect circularity, suggesting it may be slightly elongated, but broadly rounded in shape. While the majority of its light is a yellow-orange hue, there is some evidence of a slight bluer tint towards one edge, though the bulk of the galaxy's stellar population appears evolved. There is some indication of a possible minor disturbance or interaction occurring.
