The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The light distribution suggests a relatively smooth profile transitioning from the core to the outer regions, consistent with a Sersic index less than 1. The disk appears present, with slight bluer regions, possibly indicating star formation. There seems to be a small amount of dust obscuring the overall structure. The galaxy does not show any signs of tidal disturbances or major mergers.
