The galaxy presents as a system with a smooth, somewhat elongated central component. The galaxy exhibits a slight degree of asymmetry. The morphology appears to be consistent with an elliptical or lenticular galaxy, but the asymmetry could be due to minor interactions or internal structures. The color distribution suggests a slightly higher concentration of older stellar populations. The system displays some evidence of disturbance, perhaps indicating an ongoing or past interaction. Overall, it appears to be a galaxy with a generally smooth structure, but with hints of activity that warrant further investigation.
