The galaxy presents as a relatively smooth, elongated object with a slight central bulge. Its overall color appears bluish, suggesting a component of younger, hotter stars. There is a hint of asymmetry, indicating a potential disturbance or past interaction. While generally smooth, faint features or subtle undulations within the galaxy suggest a disk-like structure, though no distinct spiral arms are visible. The galaxy is not perfectly circular, exhibiting a slight elongation. There is no evidence of a major ongoing merger, though the subtle disturbances present could indicate minor tidal interactions or a previous merger event. Overall, the galaxy appears as a relatively evolved system, possibly transitioning from a spiral to an elliptical morphology, with ongoing but subdued star formation.
