The galaxy appears to be a relatively smooth, elliptical system at a moderate redshift. It exhibits a slightly elongated morphology, appearing somewhat between round and cigar-shaped. The light distribution is centrally concentrated and the color index suggests a population of older stars. The absence of prominent spiral arms or significant dust lanes indicates a lack of significant ongoing star formation. There is a suggestion of a potential minor disturbance. No clear signs of a major merger are readily apparent. Overall, the galaxy presents as a passively evolving system.
