The galaxy presents as an elongated, likely disk-shaped structure, seen at a significant angle to our line of sight. A central bulge is apparent, exhibiting a yellowish hue, potentially indicating an older stellar population and/or significant dust obscuration. Fainter, bluer regions extending from the central bulge suggest the presence of younger stars and ongoing star formation in the galactic disk. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal distortions. The overall color profile suggests a mixture of stellar populations, with a dominant older population in the bulge and a more dispersed younger population within the disk.
