The galaxy presents as a centrally concentrated spheroid, displaying a smooth, relatively featureless morphology. The core exhibits a high surface brightness, decreasing gradually toward the outer regions of the galaxy.  There is a hint of ellipticity in the overall shape. A slight color gradient is observed, with the central regions appearing whiter, suggesting a higher concentration of older stellar populations. The outer regions show a slightly bluer hue, potentially indicating some ongoing, albeit limited, star formation activity.  Faint tidal features are visible, possibly indicative of a minor merger event in the galaxy's past. The overall structure appears relatively undisturbed, although there is a non-negligible indication of morphological disturbance. There is an absence of prominent spiral arms or a well-defined disk structure.
