The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing mostly round, but with a slight elongation visible. The central region exhibits a bright, yellowish core that appears to be a bulge possibly containing an active galactic nucleus. Moving outward from the core, there is a diffuse halo or disk, which gradually fades into the background sky. This outer region displays a bluish tint, indicating the presence of some younger stars. Subtle disturbances or features may be present in the galaxy's morphology, though the image resolution is not sufficient for detailed analysis. There is a possible indication of minor tidal interactions, but there is no clear signs of major mergers or disturbances. Overall, the galaxy appears to be in an intermediate state of formation.
