The galaxy presents a generally smooth and concentrated appearance. Its morphology suggests it is primarily spheroidal in nature, with a high degree of central concentration. The light distribution exhibits a slightly elliptical shape, with no apparent spiral arm structures or prominent disk features discernible. There's a subtle color gradient within the galaxy, with the central regions appearing slightly yellower compared to the outer parts which have a fainter, bluer cast. This may indicate a concentration of older stellar populations towards the galaxy's core. There are no readily apparent signs of major merger activity or significant tidal disturbances; the galaxy seems relatively undisturbed. The size of the object is relatively compact, potentially suggesting it is an elliptical galaxy or a lenticular galaxy seen from a considerable distance.
