The galaxy presents a somewhat elliptical morphology, appearing moderately elongated in shape. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. A gradual decrease in luminosity is observed as one moves from the core to the outer regions of the galaxy. The galaxy displays a relatively smooth texture without any notable disturbances or irregularities, nor are there any significant arm structures immediately discernible, pointing to the absence of active, ongoing mergers. The color profile indicates a bias towards redder wavelengths, especially within the central bulge, which could potentially indicate an older stellar population residing there. The galaxy shows no sign of strong star formation, and has likely become more quiescent over time. The overall structure suggests a relatively evolved system.
