The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light distribution suggests an elliptical-like structure, with no apparent spiral arms or distinct disk features. The galaxy exhibits a color gradient, transitioning from a more yellow-red core to a slightly bluer, though less pronounced, outer region. The galaxy does not show signs of major mergers, though there might be subtle signs of tidal interactions or minor disturbances in its immediate vicinity. Based on the color, the galaxy has likely undergone significant star formation in the past but has relatively low levels of ongoing star formation at present. The object's shape is fairly round. The estimated mass is considerable. The galaxy is at a significant cosmological distance as indicated by its redshift.
