The galaxy exhibits a prominent spiral structure. Two well-defined spiral arms emanate from a bright, moderately sized central bulge. The arms appear relatively tightly wound near the core and gradually become more open further from the center. These arms are clearly distinguished by a bluish hue, indicating areas of active star formation. The bulge has a yellowish tint, possibly indicating older stellar populations. There is also a suggestion of dust lanes within the spiral arms, although the image resolution makes it difficult to confirm conclusively. No significant tidal features or other morphological peculiarities are immediately apparent, suggesting a relatively undisturbed evolutionary history.
