The galaxy presents as a spiral galaxy, viewed at an oblique angle. A bright central bulge is apparent, surrounded by a flattened disk structure. The spiral arms are tightly wound, appearing as faint, blueish arcs extending from the central bulge. The overall color gradient suggests an older stellar population in the bulge, with younger, bluer stars populating the spiral arms. There is no obvious indication of a strong bar structure. The morphology suggests that the central bulge is of a moderate size relative to the overall galaxy. Overall the galaxy appears well-defined, with no major disturbances or merging events readily apparent in the image.
