The galaxy presents as a somewhat symmetrical, elliptical structure. The light distribution appears centrally concentrated, exhibiting a smooth profile with a gradual decrease in intensity from the core outwards. There is no obvious spiral arm structure, and no prominent dust lanes are observed. The central region appears bright and somewhat featureless, indicating a possible bulge component. The color indices suggest a relatively evolved stellar population. There is no apparent interaction with any companion galaxies or other signs of significant tidal disturbance.
