The galaxy presents as a centrally concentrated object. The core region exhibits a high surface brightness and a nearly uniform, whitish hue. The inner regions appear relatively smooth in texture. Moving outward from the core, the galaxy displays a slightly elongated morphology, with a generally elliptical shape. There are suggestions of subtle color variations in the outer disk, with hints of redder tones along the edges. The overall impression is that of a galaxy with a dominant central bulge and a fainter, smoother disk component. There is evidence of minor disturbances in the disk region, suggesting a potential history of interaction or internal dynamic processes.
