The galaxy presents as a relatively smooth, elliptical-like structure. Its core region exhibits a concentrated, yellowish hue, suggesting a population of older stars. The outer regions display a subtle fading in intensity and exhibit a bluer tint, hinting at the presence of younger stars. The overall shape is elongated. There is no discernible spiral arm structure or strong evidence of recent major merger activity. The galaxy's morphology appears consistent with a system undergoing relatively quiescent star formation. Small disturbances and mergers are unlikely but not definitively not present. 
