The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, possibly indicative of an older stellar population. The isophotes appear relatively regular and the galaxy appears as a well-formed system. No significant signs of spiral arm structure or ongoing major mergers are visible in the image, suggesting that the galaxy has likely undergone most of its major assembly in the past and is currently relatively undisturbed. There are faint, bluish regions in the galaxy's outer areas, and a slight asymmetry in the galaxy's outer regions.
