The galaxy appears to be a relatively smooth, elliptical object with a slight elongation, exhibiting a morphology somewhere between rounded and cigar-shaped. There is little evidence of spiral arms or a prominent disk structure. The galaxy's color gradient appears to be fairly uniform, with a somewhat redder core and bluer outer regions, suggestive of ongoing, although not extremely vigorous, star formation activity, with older stellar populations dominating the core and relatively younger stars dominating the disk. There is no obvious evidence of a major ongoing merger event, but there is a slight indication of minor disturbances in the surrounding light distribution.
