The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, featureless morphology with a high degree of central concentration. The light profile is generally diffuse, with no obvious spiral arms or bar structures. The galaxy presents a yellowish-red hue, suggesting a stellar population dominated by older, redder stars and a relative lack of ongoing star formation. There may be ongoing merging occuring. The galaxy exhibits a moderate degree of roundness.
