The galaxy presents as a relatively compact object. The light distribution appears largely smooth, exhibiting characteristics consistent with an elliptical morphology or potentially a lenticular galaxy viewed at a slight angle. There is a subtle elongation. The color profile suggests an older stellar population, being redder in appearance. There is no obvious dust lane or spiral arm structure visible. Minimal tidal disturbance is apparent, suggesting a period of relative quiescence in its recent interaction history.
