The galaxy presents as a single, centrally concentrated object with a smooth, elliptical morphology. A bright, yellowish core dominates the visual appearance, suggesting a high concentration of older stellar populations. There is a noticeable decrease in surface brightness moving radially outward from the core, transitioning to a fainter, reddish halo. No distinct spiral arms, dust lanes, or prominent star-forming regions are discernible. The overall symmetrical and well-defined structure points towards a relatively relaxed and dynamically stable system. The galaxy does not show any signs of major tidal disturbances or ongoing mergers. There might be a slight flattening, but the galaxy appears largely spheroidal.
