The galaxy appears as a relatively smooth, elliptical or lenticular structure. There is a high degree of central concentration of light, suggesting an older stellar population. The color is predominantly yellow/orange, indicative of evolved stars and a lower rate of ongoing star formation. There is no distinct disk or spiral arm structure readily apparent. There are no signs of a recent major merger event or strong tidal disturbances, with the overall morphology appearing largely undisturbed. The galaxy exhibits a round shape.
