The galaxy presents an elliptical morphology. The light distribution appears relatively smooth, with a concentrated central bulge that diminishes in intensity gradually outwards. There is a slight asymmetry observed, with a hint of a possible tidal feature or minor disturbance in the halo. There are no prominent spiral arms apparent. The color profile across the galaxy seems consistent, showing no obvious regions of intense star formation. The overall structure seems consistent with a galaxy that has undergone mergers recently.
