The galaxy presents as a centrally concentrated elliptical system, exhibiting a generally smooth morphology. The core region displays a prominent luminosity, appearing nearly circular in projection. Surrounding the core is a fainter, more diffuse halo. Evidence of a potential tidal tail is visible, appearing as a minor disturbance, indicating possible past interaction or merging events. Color gradients suggest a radial variation in stellar populations, with the central region appearing redder and the outer regions showing bluer components. Overall, the galaxy appears to be a massive system, exhibiting characteristics consistent with evolved stellar populations and a relatively low ongoing star formation rate.
