The galaxy appears as a single, unresolved object. It exhibits a generally elliptical morphology with a smooth light profile, lacking any visually distinct spiral arms or bar structures. The central region is brighter and more condensed than the outer regions, suggesting a concentration of stars or an active galactic nucleus. The galaxy displays a subtle color gradient, appearing slightly bluer toward the center and redder toward the periphery. There is no obvious evidence of recent or ongoing major merger activity, although a subtle asymmetry in the outer regions may indicate minor tidal disturbances or a past interaction. The galaxy is moderately luminous, implying a substantial stellar mass and potential for ongoing star formation activity, even if not visually prominent. Overall, it seems to be a relatively evolved galaxy, possibly of early-type, at an intermediate redshift.
