The galaxy presents a generally smooth, elliptical morphology. It is characterized by a concentrated central bulge, appearing yellowish-orange, which suggests a population of older stars. The disk component appears minimal or absent, further indicating an elliptical classification. A faint, diffuse halo of bluish light surrounds the central region. There is a slight asymmetry or minor disturbance in the outer regions, but the overall structure does not appear to indicate a major ongoing merger. The galaxy displays a moderate inclination relative to our line of sight.
