The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, though a slight elongation is observed. The galaxy's core displays a bright, concentrated luminosity that gradually decreases toward the outer regions. There is a subtle color gradient visible, shifting from yellowish hues in the center to slightly redder tones in the outer regions. Some faint, diffuse features extend outward from the main body, suggesting possible tidal disturbances or interactions. The overall structure does not show any strong spiral arm presence nor bar features. There is no obvious dust lane obscuring the light from the galactic center. The galaxy seems to be isolated and relatively undisturbed, not involved in any ongoing major merger events. It is possibly a massive galaxy that is no longer actively forming stars.
