The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. It presents a concentrated central bulge of moderate intensity, surrounded by a more diffuse, extended halo. The color profile suggests an older stellar population dominating the galaxy's composition, with a noticeable lack of prominent blue star-forming regions. There is a slight color gradient, the central bulge appears more yellow, while the outer regions are somewhat redder, potentially indicating metallicity variations or differential extinction across the galaxy. There is no evidence of spiral arm structures or a prominent disk. Only minor irregularities can be observed; this might imply a past interaction or merger event. Overall, it's a well-formed and relatively quiescent galaxy.
