The galaxy presents a distinct spiral morphology. Two clearly defined spiral arms emanate from a central bulge region, exhibiting a moderate winding pattern. The galaxy’s disk appears to be viewed at a slight angle, not perfectly face-on, but not edge-on either. The central bulge region is prominent, though not overwhelmingly dominant relative to the disk. There is no strong evidence of a bar structure within the bulge. The colour gradient suggests ongoing star formation within the spiral arms, and no evidence of major mergers. Some minor disturbances might be present, but the overall structure remains largely intact. The galaxy's angular size is small but well-defined, indicating a relatively distant object.