The galaxy exhibits a generally elliptical morphology, appearing largely smooth and lacking prominent spiral arms or a distinct central bar. A bright central bulge dominates the structure, showing a concentrated, high-intensity glow. The color appears predominantly green. This suggests active star formation or a significant population of hot, ionized gas within the central region. Faint, diffuse extensions are observed surrounding the central bulge, indicating a broader halo or disk-like structure. There is a subtle suggestion of minor disturbance in the galaxy's morphology, with some asymmetry, though it is not strongly indicative of a major ongoing merger. Based on the appearance, the galaxy is likely an elliptical or lenticular type, possibly experiencing some degree of interaction or minor merger event. 
