This galaxy exhibits a generally disk-like morphology, viewed at a moderate inclination. The central region presents a bright, concentrated core. Surrounding this core is a relatively smooth, diffuse disk component. A ring-like structure is observed, encircling the central core. The ring is primarily composed of lower wavelength light, suggestive of star formation activity within. The overall color gradient of the galaxy shifts from bluer hues in the disk and core to redder tones in the outer regions, possibly indicating variations in stellar population age and composition. The light is not uniform across the galaxy, which could indicate minor disturbances.
