This galaxy presents as a somewhat smooth, centrally concentrated structure. The central region exhibits a yellowish-white hue, potentially indicating an older stellar population dominating the core. Moving outward from the core, a faint, bluish disk-like component is visible, suggesting the presence of younger stars and possibly ongoing star formation. This disk structure appears somewhat disturbed, with a subtle asymmetry or irregularity. There may be very minor signs of a faint tidal arm or disturbance at one side of the galaxy, suggesting a past interaction. The overall morphology is transitioning between elliptical and spiral. The relative color suggests moderate mass and a low star formation rate, with a specific star formation rate that is not particularly high for a galaxy at its redshift. 
