The galaxy presents as a largely homogenous, elliptical-like structure with a high degree of central concentration. The color profile appears broadly consistent, with a yellowish-white core that subtly fades into a reddish-yellow halo as one moves outward from the center. There is little to no visible substructure to suggest spiral arms or other prominent disk-like features. The overall morphology appears smooth. The galaxy has a fairly symmetric, round shape with a very faint hint of minor disturbance in its overall structure. The relatively uniform color suggests a passively evolving stellar population within this system. The galaxy appears to be a massive system, inferred from its absolute magnitude. The estimated star formation rate is low, suggesting a very low specific star formation rate.
