The galaxy presents as a concentrated, elliptical-like structure. A smooth, centrally-peaked light profile dominates its appearance, suggesting an old stellar population. The galaxy has a high degree of rotational symmetry, with a near circular morphology. There is a slight elongation visible, but no evidence of spiral arms or other distinct features such as bars or rings. The color is generally red, implying that recent star formation is minimal. No signs of tidal interactions or mergers can be seen. The light distribution is consistent with that of an early-type galaxy.
