The galaxy appears to be a somewhat elongated system, exhibiting characteristics of both an elliptical and a disk galaxy. It is not perfectly circular but exhibits an intermediate shape. The central bulge is prominent and appears relatively smooth. Faint, diffuse features suggestive of a disk are observed, although they lack well-defined spiral arms. It could be a lenticular type galaxy.

There are potentially tidal features or minor disturbances in the galaxy's morphology, especially in the outer regions, hinting at possible past interactions or mergers. The light distribution shows a gradient with a brighter core.
