The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a morphology consistent with an elliptical or lenticular type galaxy. Its overall color appears somewhat redder than average, suggesting an older stellar population with a lower rate of on-going star formation. The galaxy appears fairly isolated, lacking any strong visual evidence of major interactions or mergers, though there may be some minor disturbances to its structure. It has a slightly elliptical appearance, not perfectly circular.
