The galaxy appears to be a relatively smooth and featureless elliptical. It exhibits a high degree of central concentration, with a gradual decrease in luminosity moving outwards from the core. The overall shape is approximately elliptical but not perfectly round. There are no distinct spiral arms or a prominent bar structure visible. Color gradients suggest a slightly bluer composition in the outer regions, hinting at some ongoing star formation but this is subtle. There are no obvious signs of tidal disturbances or interactions with other galaxies. The galaxy does not appear to be a recent merger. The light profile is consistent with an older stellar population dominating the galaxy's luminosity.
