The galaxy presents as a centrally concentrated system, exhibiting a largely smooth morphology. A bright, relatively compact core region is visible, gradually fading into a more diffuse halo. The galaxy has a generally elliptical or spheroidal shape, with a high degree of roundness. There's no immediately discernible structure such as spiral arms or a prominent disk. The colour profile is dominated by a yellowish-white hue, suggesting a stellar population with a significant fraction of older stars. There is subtle bluer color in the outskirts. There is no obvious ongoing merger activity or significant tidal disturbances, however, the smoothness of the system may obscure any past interaction history.
