This galaxy appears as a single, relatively smooth object. Its morphology is predominantly elliptical. Color gradients are not apparent across the body of the galaxy, suggesting a rather uniform stellar population. There is no evidence of distinct spiral arms or a prominent disk structure. The galaxy exhibits a high degree of roundness. There are no clear signs of tidal disturbances or merger activity impacting its overall structure, though some minor asymmetry is present. The light from the galaxy is consistent with an older stellar population, suggesting relatively low ongoing star formation.
