The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. The light profile appears regular and lacks any obvious spiral arm structures or dust lanes. The color gradient suggests a redder core transitioning to slightly bluer outer regions. The isophotes appear largely round. There is no indication of ongoing major merging activity, though subtle disturbances cannot be ruled out entirely. Based on its estimated size, it's likely a massive galaxy. Star formation is present, though at a modest rate.
