The galaxy presents as a single, concentrated luminous entity, exhibiting a largely smooth and featureless morphology. It appears roughly circular in projection, with a central region of high surface brightness. The light distribution suggests a centrally concentrated spheroid, typical of elliptical galaxies or the bulge component of a spiral galaxy seen at a distance. There's a subtle color gradient, with the core appearing slightly more yellow than the outer regions, potentially indicating an older stellar population concentrated towards the center. No distinct spiral arms, bars, or dust lanes are discernible within the resolution afforded by this image, and there is no evidence of major tidal disturbances or ongoing mergers.
