The galaxy presents as a structured object with a noticeable concentration of light. Two main regions are visible: a central, bright, compact component, and an outer, more diffuse component. 

The core exhibits a bluish hue, suggesting the presence of a population of hot, young stars or significant active galactic nucleus activity. This region appears relatively smooth and unresolved.

The outer region displays a yellower coloration, which might be due to an older stellar population or the presence of dust. The overall shape appears somewhat ellipsoidal. There is a suggestion of some disk like structure, but the resolution is insufficient to confirm.

The luminosity of this galaxy implies it is a massive system. The relatively low star formation rate implied by the colors indicates that the galaxy is currently relatively quiescent, with star formation either suppressed or occurring at a low level. The disturbances reported suggest a possible minor merger event. This galaxy likely represents a massive system transitioning to a passive state.
