The galaxy presents as a generally smooth, elliptical structure. Its overall shape is close to round, exhibiting a minor deviation from perfect circularity. The light distribution appears centrally concentrated, with a fairly smooth gradient moving outward from the core. The color profile suggests a population of stars that is relatively evolved; however, there is a blue component that suggests ongoing star formation. No prominent spiral arms or bar structures are visible. There is no visual evidence of a major ongoing merger event, though some minor disturbance cannot be ruled out given the image's resolution. Based on its morphology and color, this galaxy appears to be a massive system.
