The galaxy presents as a relatively smooth, centrally concentrated system. Its morphology appears elliptical with a high degree of roundness. There is a slight color gradient, trending towards a redder hue in the central regions and bluer in the outer parts.  Evidence suggests a quiescent state with little ongoing major merging activity, although there is a subtle hint of minor disturbance in the outer regions.  It has an approximate angular size corresponding to a linear size of about 3 kpc at its redshift.
