This galaxy presents as a relatively smooth, elliptical structure. There is a concentrated central bulge, with a gradual fade in brightness toward the outer edges of the galaxy. The galaxy is not perfectly spherical. The color profile suggests a predominantly older stellar population, evidenced by the redder hues toward the center. There is some presence of bluer colors in what appears to be a faint region along one edge, potentially indicating a small amount of ongoing star formation. There are no apparent spiral arms or other disk-like features, and no obvious signs of a major ongoing merger. The structure appears relatively undisturbed. A small feature of disturbed material can be observed on the right side of the galaxy.
