The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a concentrated luminosity gradient, suggesting a high stellar density in the central regions. The overall shape is slightly elongated, not perfectly spherical, trending towards a more flattened spheroidal form. There is subtle evidence of a possible minor tidal disturbance or interaction in the form of a small disruption or plume. The primary body of the galaxy shows a homogenous light distribution.
