The galaxy presents as a system with a central, bright, and smooth component that exhibits a yellow hue. The majority of its light is concentrated here, suggesting an older stellar population within this region. Extending from the brighter central area is a fainter, more diffuse structure. This appears elongated and disk-like, with hints of bluer color, suggesting the presence of some younger stars and potential ongoing star formation. There is a slight asymmetry in the overall structure, and perhaps some minor distortion, indicating that the galaxy could potentially have experienced a past interaction or merging event. The overall smoothness of the primary light distribution suggests it is likely to be an early-type galaxy or a galaxy that has largely completed the merging process.
