The galaxy presents a generally smooth morphology, with a largely elliptical profile. The central region exhibits a high concentration of luminosity, appearing bright white. Moving outward from the core, the light smoothly transitions through hues of pink and green, indicating a complex stellar population distribution. There is minimal evidence of spiral arm structure or significant dust lanes; however, there is a very faint mottled structure on the periphery. Overall the galaxy appears as an isolated system with no close companions or signs of major recent mergers. A very slight asymmetry may indicate past interaction with a smaller satellite galaxy, or it could be an artifact of the light distribution within the galaxy itself. 
