This galaxy appears to be an elliptical galaxy, potentially of type E3-E5. It exhibits a relatively smooth light distribution, with a high degree of central concentration. The isophotes are elliptical in shape, displaying a moderate flattening, where the galaxy appears somewhat elongated. There's no evidence of spiral arms or a prominent disk structure. The galaxy's color suggests an older stellar population, lacking the bluer hues associated with active star formation. The galaxy may have had a period of low star formation, but it appears relatively quiescent at the present epoch. There is no apparent interaction with nearby galaxies, and the morphology suggests it has not undergone a major merger event recently.
