The galaxy appears to be a relatively smooth, elliptical or lenticular type. It has a centrally concentrated light profile. The galaxy exhibits a predominantly round morphology, with only slight deviations from perfect circularity. There is no strong evidence of a prominent disk structure.

The overall color gradient indicates a potentially older stellar population, with a redder central region and slightly bluer outskirts. No significant spiral arm structures are visible. There is a possibility of minor tidal disturbances or interactions, hinted at by the irregular distribution of light. However, these features are not highly pronounced, suggesting that if a merger is occurring, it is likely to be in its early stages.
