The galaxy presents as a roughly elliptical, though not perfectly spherical, object. Its core exhibits a strong concentration of light, appearing a yellow-white hue, indicative of an older stellar population. The outer regions show a more diffuse distribution of light, with subtle blue-green tinges, suggesting the presence of younger, hotter stars or regions of ionized gas associated with ongoing star formation. There is some irregular structure detected in the outer regions, which is consistent with a galaxy that could have experienced a minor disturbance. The overall morphology suggests a galaxy transitioning from a more active, star-forming phase to a more quiescent state.
