The galaxy appears as a moderately bright, elliptical or lenticular system. Its light is concentrated towards the center, exhibiting a smooth, featureless morphology without prominent spiral arms or a distinct disk structure. The overall color is slightly red, suggesting an older stellar population with relatively low levels of recent star formation. There is no sign of active galactic nuclei or other irregularities that would suggest a recent merger. The galaxy seems undisturbed and relatively isolated.
