The galaxy appears to be a relatively compact system exhibiting a predominantly smooth morphology. Its light distribution suggests an elliptical or lenticular classification. There is a strong central concentration of light. It's axial ratio is close to 1, indicating a near circular projected shape on the sky. There's no obvious spiral structure or dust lanes.

The color profile suggests the presence of an older stellar population with a hint of younger stars. The dominant light appears to be in the redder bands, with a possible trace of blue in the central parts. There may be some minor disturbances, but no major merger or violent event is apparent in the galaxy's morphology. The galaxy may be undergoing a period of low-level star formation. The color is relatively consistent.