The galaxy presents a largely elliptical morphology, appearing smooth and concentrated towards its center. It exhibits a noticeable yellow-orange hue, indicating a stellar population dominated by older, redder stars with likely little ongoing star formation. The shape deviates slightly from perfectly circular, tending towards an intermediate spheroidal form. There may be a very subtle hint of a disk-like structure present but further investigation would be required to confirm the presence of spiral arms. It does not show signs of any major mergers or significant disturbances to its overall structure.
