The galaxy presents a largely smooth morphology. Its light is concentrated centrally, fading outwards in a roughly circular pattern. The central region appears the brightest. A secondary, less luminous object is observed nearby and could suggest an ongoing or past interaction. The main galaxy exhibits a generally round profile. It does not appear to be undergoing a major merging event or exhibit significant disturbances, though a minor disturbance cannot be ruled out. The overall light profile across the galaxy appears largely uniform without prominent spiral arm structures or distinct features.
