The galaxy presents a generally elliptical morphology, appearing relatively smooth and centrally concentrated. There is little evidence of spiral arms or a distinct disk structure. The light distribution exhibits a gradual decline in intensity from the core outwards. Colors are somewhat complex and suggestive of a red shift, but also of some star formation. There might be minor tidal disturbances, but no clear signs of an ongoing major merger or interaction are immediately apparent. The galaxy appears intermediate in roundness, and is not particularly elongated.
