The galaxy presents as a largely featureless, elliptical-like structure. The core exhibits a high degree of central concentration with a yellowish hue, possibly indicating an older stellar population dominating the nuclear region. Moving outwards from the core, the galaxy gradually fades in luminosity. There's a subtle color gradient observed, shifting toward slightly redder tones in the outer regions. No distinct spiral arms or dust lanes are apparent, suggesting a lack of significant ongoing star formation. The overall morphology suggests a galaxy that has undergone significant dynamical relaxation, possibly through mergers in its past.
