The galaxy presents as a somewhat elliptical structure, exhibiting a smooth, centrally concentrated light profile. The core region is markedly brighter than the surrounding areas, suggesting a significant concentration of stars towards the galactic center. The outer regions of the galaxy appear diffuse, fading gradually into the background. The galaxy's overall color suggests a population of older stars. A faint indication of a possible tidal disturbance or interaction is present as a faint distortion in the halo. However, the signal to noise of this structure is low.
