The galaxy presents as a spiral type, although its orientation limits a detailed view of its spiral structure. The galactic disk is the dominant feature. The spiral arms appear relatively tightly wound around the galactic center. The bulge exhibits a moderate size, and the central region displays a bright, concentrated luminosity, possibly indicative of an active galactic nucleus or a dense stellar population. No significant signs of ongoing mergers or major disturbances are visible. The overall color suggests a mix of stellar populations, including younger, bluer stars within the spiral arms and older, redder stars concentrated in the bulge.
