The galaxy presents a predominantly smooth, elliptical morphology. There is a slight elongation, not quite a perfect sphere, trending towards a somewhat cigar-like shape. The light distribution is centrally concentrated. No distinct spiral arms or bar features are discernible. There is some indication of a minor disturbance in the surrounding halo, but this galaxy does not look to be in the midst of a major merger event. The color profile suggests a relatively older stellar population; bluer colors are not prominent. The low concentration of blue light indicates that the galaxy's star forming activity is suppressed.
