The galaxy presents as a spiral galaxy with a central bulge region appearing yellow-white. The spiral arms are well-defined and exhibit a tightly wound morphology. Two prominent spiral arms can be clearly identified, and there is a hint of other arm segments. These spiral arms are populated with regions of bluish light, suggesting active star formation within those areas. A faint, somewhat bar-shaped structure extends through the central bulge along the horizontal axis. There is no indication of significant morphological disturbance or ongoing major merger activity, although a possible slight asymmetry in the outer regions of the arms may suggest minor tidal interactions. Overall, the galaxy presents a classic spiral structure with indications of active star formation and a defined bulge.
