This galaxy appears to be a relatively smooth, centrally concentrated object. The light profile suggests a spheroidal morphology, with a gradual decrease in surface brightness from the core outwards. The central region exhibits a yellowish-white hue, potentially indicating an older stellar population dominating the light output. There is a subtle blueish-white halo surrounding this region. Overall, there is little evidence of distinct spiral arms or significant dust lanes. Based on its appearance and redshift, this object may be an elliptical galaxy or a lenticular galaxy. There may be a smaller galaxy that is interacting with the larger galaxy; further study should be performed. 
