This galaxy presents a generally smooth appearance. The central region exhibits a high degree of sphericity, with a concentrated, bright core that gradually fades in intensity towards the outer edges. The galaxy appears to be transitioning from a elliptical to a disk shape, slightly extended but not highly elongated. There may be minor gravitational disturbance. Although no distinct spiral arm structures are visible, there appear to be some clumpy features on its outer regions. The galaxy's color gradient transitions from yellow at its core to cooler green hues, indicating a potential variation in stellar populations, with the core potentially hosting older stellar population, and the outer regions, younger population, perhaps due to the presence of ongoing star formation.
