The galaxy presents as a relatively smooth, elliptical or lenticular structure. There is minimal visible disk component, and no evidence of significant spiral arms. It shows a moderate level of roundness. There is no strong evidence of ongoing merger activity or major disturbances in its structure. 

The galaxy exhibits a reddish hue, which indicates an older stellar population and a lower rate of current star formation. Its apparent angular size suggests it is a galaxy of moderate physical extent.
