The galaxy presents as a centrally concentrated, relatively smooth object. The overall morphology is elliptical, deviating slightly from perfect circularity. A bright central bulge is clearly discernible, surrounded by a fainter, more diffuse halo. There may be some underlying disk, but the galaxy does not display prominent spiral arms. The colour profile appears relatively uniform across the object, with a subtle color gradient from the central region outwards. There is no evidence of ongoing major merger activity, though there could be a minor tidal disturbance. Star formation rate is estimated to be low.
