The galaxy presents as a moderately bright, relatively smooth object with an elliptical morphology. The central region exhibits a higher concentration of luminosity, suggesting a prominent galactic nucleus. Moving outwards, the light gradually diffuses into a surrounding halo. There is faint hint of a disk-like structure. A subtle color gradient is observed, with the central region appearing slightly redder compared to the outer regions. No distinct spiral arms or strong dust lanes are apparent. The overall structure indicates a galaxy that is likely relatively evolved. There appears to be no significant signs of ongoing major mergers or tidal disturbances affecting the galaxy's form, although there is a faint possibility of minor interaction.
