The galaxy presents a morphology suggestive of a recent or ongoing merger. The central region exhibits a somewhat smooth appearance, though with a slight elongation or asymmetry. Spiral arm structures are not clearly defined; however, there appear to be faint, patchy areas that could be remnants of disrupted spiral features. A more detailed examination could determine if these are tidal tails or debris from the interaction with another galaxy. There is notable color variation within the galaxy, ranging from bluer regions, likely indicative of star formation, to redder regions, potentially representing older stellar populations or dust obscuration. The overall color gradient suggests a complex star formation history, possibly triggered or altered by the merger event. Overall, the galaxy displays characteristics indicative of a dynamically active system influenced by gravitational interaction. Further spectroscopic analysis would be valuable in determining radial velocities and metallicities in different regions of the galaxy.
