The observed galaxy exhibits a generally smooth morphology. The central region presents a bright, concentrated core. Moving outwards, a fainter, more diffuse halo is visible, extending beyond the core. There are some possible disturbances from external tidal sources, but the center remains largely undisturbed. The galaxy's structure seems to indicate it is potentially an elliptical galaxy. The shape of the galaxy appears relatively circular, with only slight elongation. While generally smooth, there are some hints of possible merging events or tidal disturbance, which may be influencing its overall structure. These seem to be minor disturbances however and the galaxy is not undergoing a major merge.
