The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears largely elliptical with no discernible spiral arm structure or bar. A distinct color gradient is observed, with the core region exhibiting a warmer, yellowish hue. Moving outward from the center, a subtle shift towards cooler, greenish tones is present. The galaxy is not perfectly circular, exhibiting a slight deviation toward a more flattened, elliptical form. There is no evidence of significant tidal features, strong dust lanes, or recent mergers that would suggest strong gravitational interactions. The overall morphology suggests an evolved system, potentially of considerable mass, with comparatively low current star formation activity.
