This galaxy exhibits a clear spiral structure with a relatively small bulge. The spiral arms are well-defined, with a winding pattern that appears to be somewhere between moderately wound and relatively loose. There is evidence of two main spiral arms. A bar structure seems to be present, though its strength appears to be somewhere between weak and moderate. There are signs of tidal disturbances or interactions, possibly with a nearby object, indicating a merging event may be taking place. The colour distribution suggests active star formation is occurring within the spiral arms, as indicated by the blue hues. The overall morphology suggests it is a disk galaxy viewed at a relatively face-on angle.
