The galaxy presents as a diffuse, centrally concentrated object with a somewhat elongated morphology. Its overall color appears yellowish-orange, suggesting a dominant stellar population of older stars. There may be possible disturbances or faint tidal features are observed. The galaxy's light profile is generally smooth, although there is the presence of some patchiness, possibly due to dust lanes or substructures. These observations indicate that it is likely an elliptical or lenticular galaxy. There is no strong evidence for a spiral structure, and instead, the light is distributed across a generally unstructured spheroid.