The galaxy presents as a merging system or a galaxy with significant tidal disturbances. The overall morphology is irregular and elongated. Two primary concentrations of light are visible, each exhibiting a relatively compact, bright core. These cores are surrounded by diffuse, lower-surface-brightness halos of light, giving the appearance of two interacting galaxies. The color gradient suggests a population of older stars, particularly in the tidal tails and outer regions, with some indications of younger, hotter stars within the central cores. A faint arm-like extension protrudes from one of the cores, indicating a region of potentially ongoing star formation. The galaxy appears to be relatively massive, as indicated by its luminosity and redshift.
