The galaxy presents as a somewhat diffuse, elliptical object. Its light profile appears relatively smooth and concentrated towards the center. There is a hint of radial symmetry, although the galaxy is not perfectly circular. The color index suggests a predominantly older stellar population, with a redder hue dominating the galaxy's overall appearance. There is no evident disk structure or spiral arm morphology. Faint signs of disturbance could be present, but are not readily apparent.
