The galaxy presents an overall elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a brighter, more concentrated yellowish hue, suggesting an older stellar population likely dominated by red giant stars. A fainter, more diffuse bluish component is observed, possibly indicative of a younger, star-forming region. There appear to be some signs of possible tidal disruption, with a slightly irregular shape hinting at a potential past interaction or merger event.
