The galaxy appears as a centrally concentrated, elliptical-like structure. It has a smooth morphology, lacking prominent spiral arms or bar features. The light distribution is relatively uniform with a high degree of roundness. The core exhibits the highest surface brightness, with the light intensity gradually decreasing towards the outer regions. There is a subtle color gradient visible, transitioning from a slightly bluer hue in the central region to a redder tone towards the outskirts. No significant tidal features or obvious signs of recent major mergers are apparent. The galaxy may exhibit minor disturbances indicating past interactions. Overall, it presents a quiescent appearance suggesting a relatively low star formation rate.
