The galaxy appears to be undergoing a significant merger event. The primary body of the galaxy is generally smooth in appearance, with a high degree of central concentration. The core exhibits a yellowish hue, potentially indicative of an older stellar population. Extending outwards is a fainter, bluer halo. There is an additional secondary concentration to one side of the primary body, brighter and more yellow than the halo, suggesting a second galaxy is in the process of merging. The morphology of the system is significantly disturbed, with extended tidal features difficult to discern due to the faintness, but that gives the appearance of being elongated. The merging process likely triggers elevated star formation relative to more quiescent galaxies of comparable mass, but with a small specific star formation rate. Given its apparent size and estimated distance, the galaxy is substantial.
