This galaxy presents as a relatively smooth, centrally concentrated object. The morphology is broadly elliptical, exhibiting a high degree of central symmetry. The light distribution indicates a substantial bulge component, and the galaxy's profile is smooth and centrally concentrated. The light profile appears to be well-fit by a Sersic profile, which suggests a classical bulge-dominated structure. The object's color gradients suggest a possible difference in stellar populations, with the central regions appearing redder than the outer ones. The galaxy appears to be in a relatively quiescent state with no obvious signs of recent major mergers or active star formation across most of its surface. Some subtle disturbances may be present. The galaxy is generally isolated and without any companion galaxies nearby.
