The galaxy appears to be a relatively smooth, centrally concentrated object. There is a subtle color gradient, with a slightly bluer hue in the outer regions and a redder core, suggestive of an older stellar population in the center and ongoing star formation, albeit at a low rate, in the disk. The galaxy exhibits a predominantly elliptical morphology, though with subtle deviations indicating the possibility of weak, internal disk features. There may be minor disturbance or tidal features present, potentially due to a past interaction or merger event. Overall, it presents as an intermediate-redshift galaxy with a quiescent star-formation history and some hints of dynamical activity. The galaxy's apparent size is small, which is consistent with the stated distance.
