The galaxy appears to be an elliptical or lenticular type, exhibiting a largely smooth, centrally concentrated morphology. It presents a diffuse halo of bluer light surrounding a more yellowish and concentrated core. The isophotes are generally round, showing only a slight deviation towards a more elongated shape. There is no clear indication of spiral arm structure or significant dust lanes. The overall color suggests ongoing, but relatively low, star formation activity in the outer regions. The central bulge exhibits a color consistent with an older stellar population. No obvious signs of major mergers or tidal disturbances are visible, though some minor asymmetries could indicate a past interaction or accretion event.
