The galaxy presents a generally smooth morphology, appearing relatively featureless in this image. There is an indication of a slightly elliptical shape, though it is largely rounded in its overall form. The central region displays a higher luminosity, suggesting a concentration of stars or potentially an active galactic nucleus. A subtle color gradient is present, with the central region exhibiting a yellowish hue, potentially indicating an older stellar population or a high dust content, while the outer regions appear slightly bluer, which may indicate ongoing star formation, albeit at a modest rate. There are no obvious signs of major disturbances, such as tidal tails or strong asymmetries, which suggests that it is not undergoing a major merger event, though subtle irregularities might be present at a low level. The overall appearance is consistent with that of a massive galaxy at intermediate redshift.
