The galaxy presents a predominantly smooth, elliptical morphology. The core exhibits a strong concentration of light, appearing nearly circular. The overall color profile suggests a dominant population of older stars, indicated by the yellowish hue. There is minimal visible evidence of active star formation. The galaxy's disk, if present, is not clearly defined in this image. The outer regions show a gradual decrease in luminosity without any pronounced disturbances or tidal features, implying a state of relative quiescence.
