The galaxy presents as a generally smooth, elliptical-like structure. Its color gradient transitions from a central, concentrated yellowish-white core outward to a fainter, more diffuse bluish halo. The shape exhibits a slight elongation; it is not perfectly spherical. There is no evidence of a prominent disk, spiral arms, or significant dust lanes. The light distribution suggests a relatively evolved system, potentially an elliptical galaxy undergoing low levels of star formation. No obvious signs of recent major mergers are detected, though some minor asymmetry may imply a past interaction.
