The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a high degree of luminosity, transitioning into a less intense, yet still prominent halo. The overall structure shows a high degree of roundness, with minimal apparent disruption or asymmetry. There is a subtle color gradient visible, with the central core appearing somewhat redder than the outer regions of the halo, suggesting a possible difference in stellar populations. Minimal to no spiral arm structures are apparent. The galaxy's structure suggests a relaxed system with little indication of recent or ongoing major merger events. Based on the observed characteristics, this galaxy appears to be a relatively massive system with a moderate rate of star formation.
