The galaxy presents as a complex system, likely undergoing a significant interaction or merger. It exhibits a generally smooth morphology overall, but displays distinct features indicative of disturbance. Two primary concentrations of light are observed; one is brighter and more compact, while the other is fainter and more diffuse, with a somewhat elongated shape.

There is evidence of tidal features or extended arms emanating from the fainter concentration. These appear diffuse and bluish in color, suggesting ongoing or recent star formation within these regions. The brighter concentration appears more yellow/orange in color, potentially indicating an older stellar population.

The overall color gradient suggests a variation in stellar populations and star formation activity across the galaxy. Given its luminosity and estimated size, it is likely a massive galaxy. The disturbed morphology suggests a recent interaction. Further spectroscopic analysis would be beneficial in confirming the nature of this interaction and determining the galaxy's star formation history.
