This galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a high degree of central concentration. The shape is largely round, with a slight deviation towards a more in-between, yet not quite cigar-shaped, appearance. There is a minimal indication of any major or minor disturbances, suggesting no ongoing or recent major merger events. The color gradient suggests a population of older stars. The blue, green, and red magnitudes indicate a more significant presence of older stellar populations which give it a more red appearance, with minimal recent star formation. The estimated size is relatively compact.
