The galaxy presents as a somewhat elongated, disk-like structure, viewed at an oblique angle. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or active galactic nucleus. The light distribution smoothly decreases moving away from the core. The overall color of the galaxy appears to be on the redder side, suggestive of an older stellar population and/or significant dust obscuration. The smoothness of the structure and light distribution indicates that it is likely an early-type disk galaxy. The structure is largely undisturbed, with no visual evidence of recent major mergers or tidal interactions.
