The galaxy presents a smooth, elliptical morphology. There is a concentrated central bulge that appears nearly spherical and displays a bright, yellowish-white color, suggesting a population of older stars. The outer regions of the galaxy appear less defined, with a gradual decrease in luminosity. The overall color appears redder in the central regions, which may be indicative of less recent star formation. There is little evidence of prominent spiral arms or a well-defined disk structure; the observed structure is largely spheroidal. There is a subtle suggestion of minor disturbances or asymmetries in the outer halo, possibly suggesting a past minor merger event. However, there is no indication of on-going major merger activity.
