The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round with a slight deviation towards a more elongated shape. No distinct spiral arm structures or bar features are readily apparent. The galaxy exhibits a moderately bright central region that decreases gradually in intensity towards its periphery. There are only slight suggestions of disturbances or mergers. Its stellar population appears predominantly evolved, with a color profile suggestive of older, redder stars, though the DESI magnitudes hint there is some star formation activity taking place.
