This galaxy presents as a system with an apparent disruption to its morphology, possibly indicating a merger or recent interaction. The light distribution suggests two primary concentrations of luminosity. The bluer concentration appears more diffuse and somewhat offset from the main body. A redder, more compact concentration is adjacent to the aforementioned bluer concentration. There appears to be tidal features with small disturbances, likely from gravitational interactions. The galaxy exhibits a moderate redshift, and its estimated size suggests a substantial physical extent.
