The galaxy presents an overall disturbed morphology, suggesting ongoing interactions or a recent merger event. A dominant, reddish central component is observed. A fainter, diffuse, bluish extension projects outward from this core, curving around in what appears to be a tidal feature. The blue color may indicate a region of active star formation. The central reddish component suggests an older stellar population. Faint luminosity throughout the galaxy indicates a lack of dust. This system seems to have undergone at least minor disturbances. There is faint evidence of possibly more galactic bodies near the merging galaxy.
