The galaxy appears to be a spiral galaxy, viewed at an angle closer to face-on. Distinct spiral arm structures are present, exhibiting a somewhat patchy and flocculent morphology. The arms are traced by regions of enhanced blue luminosity, indicative of recent or ongoing star formation. These regions appear intermixed with dimmer and redder portions, which may indicate older stellar populations or dust obscuration.

A central bulge is discernible. It shows a yellow-orange hue, which may point to an older population of stars. This bulge appears of moderate size relative to the overall galactic disc.

The overall structure appears to be well-formed, with no signs of major disturbance that could be indicative of a recent or ongoing merger event. There is a slight elongation in the disk, but generally, the structure seems relatively undisturbed. The galaxy's colour suggests it is transitioning, no longer vigorously forming stars, with a decreasing specific star formation rate.
