The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge, with a radial color gradient suggesting a higher concentration of older stellar populations towards the center. The isophotes appear mostly round. There may be slight indications of a disk component, or faint, diffuse features beyond the main body of the galaxy, but they are not prominent. There is no strong evidence of tidal disturbances or ongoing merger activity. Star formation seems to be low.
