The galaxy presents as a centrally concentrated object, exhibiting a generally elliptical morphology. There is a smooth, gradual decrease in luminosity from the bright, yellowish core outwards, suggesting a relatively old stellar population dominating the central region. The extended halo exhibits a more diffuse, faint blue color indicating the presence of younger stars. It is unlikely to be a strong ongoing merger event, though a minor interaction cannot be ruled out. There is a noticeable absence of defined spiral arms, however, subtle asymmetries may indicate some past interaction or disturbance. Overall, the galaxy appears to be a massive system, plausibly a relatively evolved elliptical galaxy with some ongoing star formation in its outer regions.
