This galaxy exhibits a complex morphology, likely the result of an ongoing or recent merger event. The central region displays a concentrated luminosity. The galaxy appears to be undergoing significant interaction, possibly with another galactic body, based on its disturbed morphology. There is some suggestion of tidal tails, possibly from ejected material, however, the limited resolution makes that difficult to say for sure. Color analysis suggests a mixture of stellar populations, including possibly regions of intense star formation alongside older, redder components. The general shape is roughly rounded, but with significant deviations due to the interaction. The presence of both disturbed features and high redshift suggest a relatively early stage in its evolutionary timeline.