This galaxy presents as a smooth, somewhat elliptical structure. The central region exhibits a concentrated and relatively bright, yellowish core, suggesting a substantial population of older stars. The luminosity decreases gradually outwards from the center, with a redder hue toward the outer edges of the galaxy. The shape is largely spheroidal, although subtle irregularities may indicate minor disturbances in the galactic structure, the overall appearance is relatively undisturbed. There is no strong evidence of spiral arms or a prominent disk component. The light distribution suggests a fairly high degree of symmetry.
