This galaxy presents as a relatively smooth, elliptical-like structure. The light is concentrated toward the center, suggesting a high density of stars in the galactic nucleus. There is some indication of a slight disky component or faint features present. The galaxy exhibits a bluer hue near the core, possibly indicating ongoing star formation. The outer regions fade gradually, showing little evidence of distinct spiral arms or prominent features. Overall, the galaxy seems to be in a relatively quiescent state, with no major disturbances or merger activity readily apparent.
