The galaxy appears as a fairly symmetrical, elliptical structure. Its overall color profile indicates a dominance of older stellar populations, suggesting a relatively low rate of current star formation. The core region is notably brighter and appears yellower, which could indicate a higher concentration of evolved stars or dust obscuration within that central area. There is a faint, diffuse halo surrounding the core, gradually fading into the background sky. No distinct spiral arms or prominent dust lanes are discernible, reinforcing the classification as an elliptical galaxy. The galaxy's smoothness suggests it is likely undisturbed, without any major ongoing merging events. The overall round shape further supports its classification as a relatively relaxed system, potentially close to dynamical equilibrium.
