The galaxy presents a morphology suggestive of a system undergoing a merging event. The overall structure appears amorphous, lacking a well-defined spiral or elliptical shape. There are at least two distinct, bright core regions, which may indicate the presence of two galaxies in the process of merging. These cores exhibit a yellowish-white hue, suggesting an older stellar population. Faint tidal tails or bridges of material extend from the central regions, indicating gravitational interaction and disruption. There is a hint of bluer regions within the fainter outer regions, possibly indicating areas of recent star formation triggered by the merger. The system appears relatively smooth overall. The morphology indicates that this galaxy is not at equilibrium but is actively evolving.
