The galaxy presents as an elliptical form, elongated in shape, with a smooth, relatively featureless structure. The central region exhibits a bright, concentrated luminosity, suggestive of a dense stellar population or active galactic nucleus. Moving outwards from the core, the light gradually diminishes, displaying a radial profile consistent with a bulge-dominated system. Subtle color variations are observed, with a yellowish hue dominating the core, potentially indicating an older stellar population. Fainter, bluish tinges are perceptible in the outer regions, hinting at the presence of younger stars or ongoing, albeit subdued, star formation. There is no clear evidence of spiral arms or a distinct disk structure. The overall morphology suggests a relatively evolved galaxy, likely an elliptical or lenticular type, undergoing limited present-day star formation.
