The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light profile with a high degree of symmetry. The central region is bright, with a yellowish hue suggestive of an older stellar population. Fainter, more diffuse light extends outwards from the core. There are some indications of features or a disk-like structure. The outer regions exhibit some level of disturbance. The galaxy's shape is approximately round. This object shows evidence of possible past or ongoing interaction with another galaxy.
