The galaxy appears as an elliptical system, exhibiting a smooth, concentrated morphology. Its overall shape is predominantly round, with only a slight deviation towards ellipticity. The light profile indicates a centrally concentrated bulge that is approximately 4.8 kpc in radius. The central region is yellow, suggesting an older stellar population. The faint halo surrounding it extends further, showing a very subtle gradient in color suggesting an overall diminishing population of older, redder stars, but with limited, if any, recent star formation. There is no visible dust lane or spiral arm structure present. There are no signs of tidal disturbances or ongoing mergers.
