The galaxy presents as a slightly inclined spiral, displaying a substantial disk component. Spiral arms are discernable, though somewhat tightly wound and not sharply defined. The central bulge is present, exhibiting a moderate size relative to the overall disk. There may be a subtle bar structure, though it is not distinctly prominent. There is no evidence of any major merging or disruptive interactions with other galaxies. The overall color suggests active star formation with a stellar mass on the larger end.
