The galaxy appears as a single, centrally concentrated object. Its morphology seems largely smooth, with a nearly round appearance, though it's not perfectly spherical. There is little evidence of spiral arms or a disk-like structure. A subtle color gradient is observed, with the central region possibly exhibiting a slightly redder hue compared to the outer regions, potentially indicating an older stellar population concentrated toward the center. The galaxy displays a moderate redshift. Based on the observed color and structure, this galaxy is likely a relatively massive system with suppressed star formation. There is no evidence of major mergers or strong tidal disturbances, suggesting a relatively isolated evolutionary path. The galaxy's luminosity appears moderate, falling within typical values for galaxies at its redshift.
