The galaxy presents as a spiral type, exhibiting a defined disk structure. Evident spiral arms emanate from a central bulge, which comprises approximately 30-50% of the galaxy's total size. A bar is present at the center of the galaxy, and it is weak. No significant mergers are present, and the galaxy appears undisturbed. Star formation is present, and the galaxy has intermediate stellar mass. The galaxy is inclined at an angle and is not viewed edge-on.
