The galaxy presents as a centrally concentrated system with a smooth overall appearance. It exhibits a predominantly elliptical morphology, appearing nearly round with only a slight elongation. The core region is noticeably brighter and exhibits a reddish hue, possibly indicating an older stellar population. Moving outward from the core, the color shifts towards a more greenish-yellowish tint, suggestive of ongoing, though perhaps modest, star formation. No distinct spiral arms or strong tidal features are apparent in this image, though a subtle, low-contrast disk-like structure might be present surrounding the bulge. There appears to be a hint of minor disturbance to the shape, as a slight asymmetry is visible in the outer regions of the galaxy. Overall, the galaxy appears to be a massive system, likely located at a substantial cosmological distance.
