The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular system. It exhibits a subtle color gradient, transitioning from a slightly bluer hue in its outer regions to a redder, more pronounced core. The galaxy appears to be fairly rounded in shape. There may be some indication of minor tidal disturbances present, but this is difficult to ascertain with certainty given the resolution. A substantial portion of the galaxy's light is emitted from an older stellar population, as evidenced by its redder color. Despite the smooth appearance, a small portion of the light emitted is from younger stars. The system shows an estimated diameter of roughly 5 kpc. There is an indication it may be in the process of a minor merger event.
