The galaxy appears as a bright, centrally concentrated object with a smooth, yellowish-white core. It exhibits a somewhat elliptical morphology, with the luminosity decreasing gradually from the center outwards. A faint, bluish extension is visible on one side of the galaxy. This feature suggests the presence of a tidal tail, likely the result of a past interaction or merger event. There is no apparent spiral structure or distinct disk. The overall appearance suggests an older stellar population dominating the central regions, while star formation is more active in the tail. Based on these characteristics, the galaxy is likely to be a massive, relatively evolved system.
