The galaxy presents a smooth, centrally concentrated morphology. It exhibits an elliptical or lenticular structure, with a high degree of radial symmetry. The light distribution suggests a dominant spheroidal component. There is no evidence of spiral arms or a well-defined disk. The galaxy appears yellowish-white in color, indicating an older stellar population with a lack of significant ongoing star formation. Its moderate luminosity, combined with its smooth appearance, is consistent with it being a relatively massive galaxy. The shape is slightly elongated. There are no clear signs of tidal disturbances or interactions with other galaxies.
