The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears largely elliptical, exhibiting a high degree of roundness. There is a discernible color gradient, transitioning from a yellowish-orange core to a bluer, diffuse outer halo. No distinct spiral arm structures or prominent dust lanes are apparent. The overall structure suggests a lack of recent major merger events. The luminosity profile indicates a centrally dominant core with a gradually decreasing surface brightness outward. Based on the color and lack of distinct features, the galaxy appears to be a relatively massive system with modest star formation.
