The galaxy appears to be a somewhat elliptical structure, exhibiting a smooth, centrally concentrated light profile. Its core is a bright, yellowish-white color, suggestive of an older stellar population. Fainter, slightly bluer regions extend outwards from the core, indicating the potential presence of some younger stars or ongoing star formation. There is some evidence of a possible minor disturbance in the morphology, perhaps a faint tidal tail or asymmetry suggesting a past interaction. The galaxy is not perfectly round; its shape is somewhat elongated. There appears to be no active merger occuring at present. The galaxy has a red shift value, which indicates it is a distant galaxy. The galaxy appears to be of moderate size and mass. Overall, the galaxy presents a morphology that blends characteristics of an elliptical galaxy with hints of more recent star formation and possible minor interactions.
