The galaxy presents a generally smooth appearance, although the color distribution hints at some underlying structure. The central region appears bright and concentrated, suggesting a possible bulge or core. There is a slight elongation or flattening of the galaxy's shape, indicating it may be a disk galaxy viewed at an angle rather than a perfect elliptical. There is some asymmetry in the galaxy's outer regions, with one side appearing slightly more extended or distorted than the other, suggesting a possible interaction or minor disturbance. Overall, the galaxy's structure does not strongly indicate a major merger event.
