The galaxy presents a largely smooth and elliptical morphology. It exhibits a centrally concentrated luminosity profile. The core region displays a yellowish-white hue, suggesting a population of older stars and minimal on-going star formation. The outer regions display a radial color gradient, becoming slightly redder in appearance with increasing distance from the center. There appears to be minimal evidence of spiral arms or distinct structural features. There is no apparent ongoing merger activity. The galaxy appears to be a relatively isolated system.