The galaxy presents as a relatively small spiral, with a prominent disk structure. Evident spiral arms extend from a faint central bulge. The winding of the spiral arms appears to be generally medium, with elements of both tighter and looser morphologies. There is an indication of a two-armed spiral structure, however, this is hard to confirm. The galaxy demonstrates a bluer color profile, suggesting active star formation within the spiral arms. While the disk is not perfectly edge-on, it is near enough to allow observation of both sides. The spiral arms exhibit some clumpy regions, potentially indicating HII regions or star clusters. There is no clear evidence of a strong bar structure, but there is no evidence against a weaker one. The galaxy exhibits some signs of disturbance or minor interactions.
