The galaxy presents as a centrally concentrated object with a diffuse, extended halo. The central region exhibits a bright, compact core, suggesting a concentration of older stellar populations.

The overall color profile appears to be relatively uniform, with a slight bluer hue in the outer regions. It shows a smooth and relatively featureless morphology, lacking apparent spiral arms or bar structures. The shape appears generally elliptical or nearly circular. There is no evidence of major tidal disturbances or ongoing mergers. There might be some signs of a minor interaction or internal disturbance to the morphology of the galaxy.
