The galaxy appears to be a spiral galaxy, oriented at a slight angle relative to our line of sight. The disk is visible, showing distinct spiral arm structure. Two prominent spiral arms emanate from a central bulge region. The arms appear relatively tightly wound.

The central bulge region presents a yellowish-white hue, suggesting an older stellar population. The spiral arms exhibit a bluer color, indicative of ongoing star formation. The galaxy's overall structure suggests a moderate bulge size. There's a potential sign of a weak bar structure present in the central region of the galaxy. The galaxy shows no major disturbances in its morphology, and it's likely not undergoing a major merging event. There could be some indications of a minor disturbance, though.