The galaxy appears to be a relatively smooth, elliptical galaxy. The light is concentrated toward the center, indicating a prominent bulge. The galaxy has a moderate axis ratio, and a slightly elongated shape, appearing somewhere between round and cigar-shaped. There is no clear evidence of strong spiral arm structure or major disturbances, though a faint hint of an outer disk. The color profile exhibits a gradient, with the central bulge appearing more yellowish-white, possibly indicating an older stellar population and/or dust obscuration. The outer regions appear slightly bluer suggesting the presence of younger stars, though in relatively small quantities. No obvious signs of ongoing merging activity are detected.
