The galaxy presents as an elliptical form, with a smooth and concentrated central bulge. The luminosity appears to gradually decrease from the core outwards. The color profile suggests an older stellar population, evidenced by the redder hues dominating the central regions. There is no distinct spiral arm structure visible, and the outer regions appear relatively uniform in color and texture. There is a very slight indication of a disk. No signs of active galactic nuclei, tidal disturbances, or ongoing major mergers are apparent from this image. The galaxy displays a high degree of symmetry.
