The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. The core appears bright and yellowish, suggesting an older stellar population. The galaxy exhibits a diffuse outer halo which fades into the background. There appears to be no prominent disk structure or spiral arms. There may be minor tidal disturbances or asymmetries in the outer regions, but the dominant impression is one of a relatively undisturbed, relaxed system. The overall color gradient indicates a redder population towards the center and bluer population in the outer regions, which suggests ongoing star formation is occurring.
