The galaxy presents an ellipsoidal morphology with a smooth, mostly featureless appearance. The light profile suggests a centrally concentrated structure. The galaxy exhibits a warm color, tending toward redder wavelengths, indicative of an older stellar population or significant dust obscuration. Faint tidal features and irregular shapes suggest this galaxy is likely undergoing a merger, but this disturbance is not easily visible without further image processing. There is not much evidence for ongoing star formation.
