The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology suggests an elliptical or S0 type galaxy. The core exhibits a bright, yellowish hue, which likely indicates an older stellar population. There is a slight asymmetry in the light distribution, perhaps a hint of faint tidal features or subtle disturbances indicating a possible past interaction or merger. A patch of redder color on one side indicates the presence of either a slightly redshifted population of stars in that region, or perhaps a dust lane obscuring a bluer population. Overall, the galaxy presents a mature, largely quiescent appearance.
