The galaxy presents a largely smooth, elliptical morphology with high degree of central concentration, appearing mostly round. The color gradient indicates a relatively old stellar population, exhibiting a reddish-yellow hue across its entirety, with very little if any blue color indicative of on-going star formation. There is no observable disk structure or spiral arms. No apparent signs of tidal disruption or major merger events are present. Based on color, overall form, and smoothness, the object is likely a spheroidal galaxy with minimal recent star formation.
