The galaxy presents as a flattened elliptical, likely a disk galaxy viewed at an oblique angle. Its core exhibits a concentrated, bright, yellowish-white hue, suggestive of an older stellar population and potentially a supermassive black hole. Proceeding outward, the central region fades smoothly into a more diffuse disk. This disk displays a subtle gradient, transitioning from the yellowish-white center to a reddish-orange periphery, hinting at ongoing or recent star formation. Faint bluish regions can be discerned, possibly indicative of younger, hotter stars. No clear spiral arm structure or bar feature is readily apparent. The overall morphology appears largely undisturbed, lacking any obvious signs of major mergers or tidal interactions.
