The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a concentration of light towards the center, suggestive of a bulge. The galaxy appears largely undisturbed, with no obvious tidal features or signs of recent major mergers. The light profile indicates a galaxy that is neither perfectly spherical nor highly elongated. There may be some minor internal asymmetry, but no strong evidence of spiral arms or a prominent disk structure is visible. The color suggests an older stellar population, possibly indicating that star formation is either low or absent.
