The galaxy presents a distinct spiral morphology, viewed at a near edge-on inclination. Two prominent spiral arms are visible, loosely winding from a central bulge. The bulge appears relatively small compared to the overall disk size. The spiral arms exhibit a clumpy structure, suggesting active star formation regions. The disk is slightly asymmetric, possibly indicative of minor gravitational interactions. The galaxy displays a blue hue, particularly within the arms, indicating a younger stellar population. A faint bar structure seems to traverse the central region. There are no signs of tidal tails or major disturbances. The color appears bluer in the spiral arms.
