The galaxy presents as a centrally concentrated system with a largely smooth morphology. The primary color component is yellow/orange, which suggests an older stellar population dominating the light output, indicative of reduced star formation activity. There is a slight elongation visible in the galaxy's overall shape, and it appears nearly round. No distinct spiral arms or bar structures are discernible. There are no indications of any recent or major merger events based on its regular and undisturbed morphology. It is potentially an elliptical galaxy, but the resolution does not allow definitive classification. 
