This galaxy exhibits an elliptical morphology, appearing relatively smooth and well-defined. There is a prominent central bulge, characterized by a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the galaxy's color subtly shifts towards a bluish-white, indicative of younger stellar populations and possible ongoing or recent star formation. There are hints of a faint disk-like structure, though it is not sharply defined. The overall appearance suggests a system that may have undergone past interactions or minor disturbances, without significant disruption to its overall structure. The shape is generally round, with a slight elongation. Evidence of any major mergers is not immediately apparent.
