The galaxy presents a largely smooth morphology, exhibiting a predominantly elliptical shape with a high degree of roundness. A central bulge is clearly visible, appearing bright and concentrated. A faint disk may be present, but the image resolution makes it difficult to determine a spiral structure. There is no prominent evidence of ongoing mergers or major disturbances in the galaxy's morphology. Based on the blue color, there is likely a relatively moderate amount of ongoing star formation within the galaxy.
