The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its overall form is moderately rounded, exhibiting a slight elongation along one axis. There is little evidence of spiral arms or significant dust lanes. The light is dominated by redder wavelengths. Star formation appears to be generally suppressed, with a low specific star formation rate. The galaxy appears to be quite massive, likely exceeding 10^11 solar masses. There is no indication of an ongoing major merger, although potential minor disturbances cannot be entirely ruled out.
