The galaxy appears to be a relatively smooth, elliptical galaxy, likely at an intermediate redshift. Its overall form presents a fairly regular, rounded profile with no obvious signs of strong tidal interactions or major disturbances. There is a gradual decrease in luminosity from the galactic center outwards. The core region is distinctly brighter and exhibits a slightly yellow-white hue, suggesting the presence of an older stellar population. The outer regions of the galaxy gradually fade into the background sky, showing a blueish tint potentially indicative of a small amount of ongoing, although limited, star formation, or from being further away in the galaxy's structure. No distinct spiral arms or prominent dust lanes are observed, which further supports the classification as an elliptical galaxy. The image does not reveal any significant structural features like bars or rings. Overall, the galaxy presents a well-defined but non-complex morphology.
