The galaxy presents as a relatively small, well-defined spiral galaxy exhibiting a clear disk structure. The spiral arms appear well-formed, with a moderately open winding. Two distinct arms are discernible, suggesting a grand design spiral morphology. There is no noticeable bulge component at the center of the galaxy; rather, the central region appears diffuse and subtly elongated, possibly indicative of a weak or non-existent bar structure. The overall color profile indicates active star formation across the disk, most notably in the spiral arms. Some of the features are somewhat disturbed, suggesting some possible ongoing gravitational interactions with a minor merger or minor tidal disturbance with another galaxy. The galaxy is not viewed edge-on.
