The galaxy presents as an elliptical or lenticular type. The light profile is generally smooth and centrally concentrated, with a noticeable elongation suggesting an ellipsoidal shape viewed from an angle. The central region exhibits a yellowish-white hue, potentially indicative of an older stellar population. Surrounding this central region, there is a fainter, bluer component suggesting the presence of younger, hotter stars. This bluer component appears more diffuse. There is a slight asymmetry in the outer regions, but no clear evidence of major tidal disturbances or ongoing mergers. The galaxy does not display prominent spiral arms.
