The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a subtle color gradient, appearing slightly bluer towards the core and gradually becoming redder in the outer regions. This color distribution suggests a population of older stars dominating the outer regions, with a possibly younger, hotter stellar population concentrated in the galactic center. The apparent lack of distinct spiral arm structures further supports its classification as a galaxy transitioning into or already existing as a fairly passive and evolved system. Overall the morphology indicates low star formation.