The galaxy presents a clear spiral structure. Spiral arms are tightly wound, showing a relatively ordered configuration. The central bulge appears moderately sized, exhibiting a yellowish hue, which suggests an older stellar population. A bar structure may be present, but is not strongly defined. The disk component is the dominant feature, and is oriented nearly face-on. The spiral arms are not well resolved into individual star-forming regions. The color gradient from the center to the outer disk indicates a possible decrease in stellar age and metallicity with increasing radial distance from the nucleus. There is no visible evidence of major mergers or significant disturbances in the galaxy's morphology.
