The galaxy exhibits a largely smooth morphology. A central bulge is visible, appearing relatively bright and concentrated. The overall shape is generally round, with minimal elongation or asymmetry. There are subtle features suggesting some minor disturbances in the outer regions of the galaxy, but no major distortions or clear signs of an ongoing merger. The color appears to be a slightly redder hue, suggesting an older stellar population. Star formation appears to be low, but present. 
