The galaxy presents a generally smooth, elliptical morphology, with the majority of its light concentrated towards the center. There is a slight elongation present, but the galaxy is relatively round. A bright central bulge is clearly visible, surrounded by a fainter, more diffuse halo. Colors indicate a generally older stellar population, with a hint of younger stars in the outer regions, possibly indicating some ongoing, albeit low-level, star formation. There is no evidence of strong tidal disturbances or major mergers, although there might be a very faint indication of a minor interaction in the outer halo. The overall structure appears relatively undisturbed.
