The galaxy presents a largely smooth morphology. Some faint irregularities or disturbances are suggested within its structure, though they do not indicate a major ongoing merger. The galaxy appears to be a primarily smooth object. A slight asymmetry or subtle distortion is possibly evident, hinting at a potential past interaction or minor merger event, which could be a disturbance. The galaxy's light distribution exhibits a noticeable color gradient, becoming redder towards the central region, which implies varying stellar populations. It has a compact appearance with a relatively high surface brightness.
