The galaxy presents with a centrally concentrated, smooth morphology, exhibiting a largely elliptical shape. The core region displays a notably brighter, more intense orange hue, suggesting a higher concentration of older stellar populations. The outer regions show a gradual decrease in luminosity, transitioning to a fainter, more diffuse glow. There's a subtle hint of disk-like structure, but no clear spiral arms or distinct features are readily apparent. No major signs of tidal disturbances or mergers are observed, though a minor asymmetry or irregularity cannot be entirely ruled out at this resolution. The overall color gradient indicates a possible decline in star formation rate from the central regions outwards.
