The galaxy presents as an elongated, disk-like structure viewed nearly edge-on. It exhibits a central bulge that appears relatively smooth and concentrated. The disk component displays a bluish hue, suggesting the presence of ongoing star formation activity. The galaxy's light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer edges of the disk. There are no immediately apparent signs of strong tidal disturbances or major mergers, although some minor irregularities in the disk's structure cannot be ruled out. The overall morphology suggests a relatively undisturbed, rotating disk galaxy with moderate star formation.
