This galaxy exhibits an elliptical morphology, appearing largely smooth with a concentration of light towards the core. There is a slight elongation present, deviating somewhat from a perfectly circular profile, but it is mostly somewhere between round and oval. I can only see hints of spiral arms or other disk-like features. The color gradient suggests that the central region is more abundant in older, redder stellar populations. There may be a small amount of active star formation occurring in the outer parts of the galaxy, with a small amount of blue light present. Overall, it appears to be relatively undisturbed, showing no obvious signs of ongoing mergers.
