The galaxy presents as a luminous, disk-shaped structure with a noticeable bulge. Its orientation appears tilted with respect to our line of sight, suggesting it is not perfectly face-on. The central bulge region exhibits a high surface brightness, indicative of a concentration of older stellar populations. Moving outward from the center, the disk shows a gradual decrease in surface brightness. The color gradients suggest that the inner regions are relatively redder. It has a notable star forming region throughout. The galaxy appears relatively isolated with no obvious signs of a major ongoing merger event, although there might be minor disturbances in the disk morphology.
