The galaxy presents an overall elliptical morphology, appearing somewhat flattened. The central region exhibits a high surface brightness, suggesting a concentrated nucleus. Moving outwards from the core, the galaxy displays a gradual decrease in luminosity, characteristic of an elliptical galaxy. The color profile indicates a predominantly older stellar population, with a subtle blue tint in the outer regions, potentially indicating some degree of recent or ongoing star formation, this is potentially coming from a disk or featured structures in the galaxy. There may be evidence of a minor disturbance to the overall galaxy shape.
