The galaxy presents as a relatively smooth and centrally concentrated structure. The light distribution exhibits a high degree of symmetry, with a near-circular isophotal shape. There is a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a redder, more luminous core. The overall appearance suggests an evolved system, potentially an elliptical or lenticular galaxy, with a dominant bulge component and minimal evidence of spiral arm structures or significant dust lanes. The morphology indicates that the galaxy is likely a relatively relaxed system, undisturbed by recent major mergers. The small amount of blue light could suggest there is some minor star formation.
