The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution appears fairly uniform and centrally concentrated. The color index, judging from the RGB bands, indicates a redder stellar population; suggesting older stars dominate the galaxy's composition. There is no evidence of spiral arms or significant dust lanes. There is no significant morphological disturbance, but a possible minor asymmetry or disturbance within the galaxy's halo structure cannot be ruled out given the image quality, but the galaxy generally appears to be a settled system.
