The galaxy presents as a single, relatively compact object. It exhibits a dominant, smoothly distributed light profile, suggesting an elliptical morphology, though some deviation from perfect circularity is noted, tending towards a more elongated shape. Its color indices indicate the presence of an older stellar population, with a bias toward redder wavelengths, and a hint of some bluer stars. There is no obvious spiral arm structure or prominent dust lane obscuration. There is little evidence of strong ongoing star formation. It appears to be isolated, without any major signs of an ongoing merger or significant tidal disturbances.
