The galaxy presents a generally smooth morphology. It appears elliptical in shape, with a slight elongation along its major axis. A dominant central bulge is evident, exhibiting a concentrated, bright yellowish glow. There is a subtle color gradient from the center outwards, the outer regions appearing somewhat bluer than the core, suggesting the potential for some low-level star formation in the outer regions. There is no obvious spiral structure. Based on the lack of substantial disturbance and the smooth nature of the galaxy, it is unlikely to be undergoing a major merger. Minor disturbances cannot be ruled out completely.
