The galaxy presents as a centrally concentrated structure with an overall elliptical morphology. It displays a smooth light profile, suggesting it is primarily composed of older stellar populations with a minimal disk component. The core exhibits a brighter, more intense luminosity, potentially indicative of a supermassive black hole or a dense stellar nucleus. There appears to be some minor asymmetry, but no clear tidal features or signs of a major ongoing merger. The galaxy's color suggests moderate star formation or an older population.
