The galaxy appears to be a luminous, elliptical system. Its morphology is largely smooth, with a high degree of central concentration. The overall color profile exhibits a radial gradient, with the core displaying a yellow-orange hue, suggestive of an older stellar population dominating the central regions. The outer regions show hints of bluer tones, potentially indicating the presence of a younger stellar population and ongoing star formation, albeit at a lower rate. The shape is predominantly round, showing little to no disc structure or indication of spiral arms. There is no apparent evidence of tidal features or recent major mergers. Subtle asymmetries or minor disturbances may be present, but they are not a dominant characteristic of its overall structure.
