The galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction. A dominant, centrally located, bright component displays a somewhat smooth appearance, though with hints of substructure or possibly tidal features extending from it. This primary component shows a slightly bluish hue.

Adjacent to this is a fainter, more elongated structure exhibiting a yellowish color gradient. The spatial proximity suggests a possible tidal interaction or merger with the brighter, more compact galaxy. The overall extent of the system is relatively compact, and appears to be more than 7 arcseconds in diameter.

There is some evidence of minor disturbances in the structure of the galaxy. While a significant portion of the galaxy appears smooth, there are also indications of potential disturbances possibly caused by an ongoing merger.
