This galaxy appears to be a relatively small, early-type galaxy, exhibiting a smooth, elliptical morphology. It presents a concentrated central bulge, with stellar density decreasing radially outward. The galaxy appears to be generally round. The galaxy color indices suggest a redder, more evolved stellar population, characteristic of galaxies with low current star formation rates. The apparent lack of spiral arm structure or prominent dust lanes further indicates a quiescent or post-starburst system. There is no prominent ongoing merger activity, although some minor disturbance cannot be ruled out. The overall appearance points to an elliptical galaxy or a lenticular galaxy with a dominant bulge and faint disk.
