This galaxy presents a spiral morphology, with a disk that is neither perfectly face-on nor edge-on to our line of sight. The disk exhibits distinct spiral arms, primarily displaying a two-armed structure. These arms show a medium winding tightness. The galactic bar is present. The central bulge appears moderately sized, contributing significantly to the galaxy's overall luminosity. Within the disk, there are regions exhibiting a bluer hue, suggestive of active star formation. The galaxy is relatively isolated, however the morphology suggests a recent or ongoing interaction or disturbance event. 