The galaxy presents as a spiral type. It exhibits a prominent central bulge with a yellowish hue, suggesting an older stellar population in this region. A distinct bar structure bisects the bulge, appearing relatively strong. The spiral arms emanating from the bar are tightly wound and show a bluish tint, indicative of ongoing star formation. Two dominant spiral arms are readily discernible. While not perfectly symmetrical, the disk component is well-defined. There's no apparent sign of tidal disturbance, such as extended streams or distorted morphology, and no evidence of a major merger event. 
