The galaxy presents as a luminous, elliptical or lenticular system. The galaxy exhibits a smooth, concentrated light profile with a fairly round morphology, suggesting a relatively relaxed dynamical state. A slight elongation is present, hinting at a weak bar or possibly tidal interaction. The color is predominantly yellowish, suggesting an older stellar population with minimal ongoing star formation. There are no apparent spiral arms or dust lanes visible, supporting the hypothesis of an elliptical or lenticular classification. There is a possible interaction with another galaxy that is seen at a closer proximity, this may be disrupting its shape. The system is moderately large, indicating a substantial stellar mass.
