The galaxy exhibits a generally elliptical morphology, appearing mostly smooth in structure. The central region displays a concentrated brightness, suggesting a prominent galactic nucleus. The color profile shifts from a warmer, more yellowish-orange hue at the core to cooler, slightly greenish tints in the outer regions. There is little evidence of strong spiral arm structures or significant dust lane obscuration. The overall appearance indicates a relatively evolved system, likely a massive galaxy with a moderate rate of star formation. Subtle irregularities in the outer regions might hint at minor gravitational disturbances or past merger events, though the dominant impression is one of a largely undisturbed, mature galactic form.
