The galaxy presents a largely smooth, elliptical morphology. The color profile indicates a concentration of older stellar populations, with a central bulge exhibiting a yellowish-orange hue. Fainter, bluer light emanates from the outer regions, suggesting the presence of some younger stars, possibly within a faint, diffuse disk. The overall roundness suggests a relatively low inclination. There is no obvious evidence of any major ongoing merger activity, although minor disturbances might be present in the faint outer reaches of the galaxy. The galaxy's integrated light appears to be dominated by evolved stars, and the rate of star formation appears to be low. The estimated mass of the galaxy is substantial.
