The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. There is no apparent spiral structure or distinct features such as bars or rings. The light profile appears roughly elliptical, tending toward a circular shape.

The core exhibits a higher surface brightness, fading gradually into the outer regions. A slight color gradient is discernible, with the central region displaying a warmer hue. The outer regions of the galaxy are considerably fainter and appear bluer in color. There is no visual evidence of ongoing major mergers or tidal disturbances. The overall appearance suggests a relatively evolved system with a dominant bulge component and potentially a weak or non-existent disk.
