The observed galaxy presents a clear spiral morphology. Two distinct spiral arms are visible, exhibiting a moderate-to-loose winding. The central bulge appears relatively small. The disk is not perfectly edge-on, allowing a clear view of its spiral structure. Indications of active star formation regions are evident within the spiral arms, exhibiting a bluer hue than the surrounding stellar population. No major tidal disturbances or evidence of an ongoing major merger are apparent, though some minor irregularities in the spiral arms suggest a possible past interaction or minor disturbance. A weak bar structure may exist in the center of the bulge, but the evidence is not definitive. Overall, the galaxy seems to be a relatively undisturbed spiral galaxy, with a moderate amount of ongoing star formation in its arms.