The galaxy presents a largely smooth and centrally concentrated morphology. The light profile appears to diminish gradually from the core outwards, with no apparent spiral arms or distinct features discernible in the observed wavelengths. It appears to be primarily a spheroid galaxy, with a slight elongation. There is a faint blue color, suggesting some ongoing star formation activity within the galaxy, although it is relatively weak. No major signs of mergers or tidal disturbances are apparent in this image. Overall, the galaxy presents as a relatively undisturbed system.
