The galaxy presents as a moderately inclined, elongated disk. Its color is primarily reddish, suggesting a dominant population of older stars and potentially significant dust obscuration. There is a subtle hint of structure within the disk, but no prominent spiral arms are discernible. The galaxy appears to be relatively isolated, showing no obvious signs of major tidal disturbances or ongoing mergers. It exhibits a smooth overall appearance. The axial ratio suggests a shape deviating significantly from a perfect circle. 
