The galaxy appears to be a disk galaxy, viewed at a high inclination, possibly close to edge-on. The central bulge is bright and concentrated, exhibiting a strong emission, potentially indicating an active galactic nucleus or intense star formation. The disk is relatively thin and elongated. There are faint spiral arm structures visible within the disk, although they are not well-defined, implying a flocculent or loosely wound spiral morphology. The color of the bulge appears to be more yellow-white, suggesting an older stellar population. The disk shows hints of bluer regions, likely indicating younger, hotter stars and star-forming regions. There's a subtle distortion or possible tidal feature extending, which could be evidence of a past or ongoing interaction with another galaxy, albeit a minor one. Overall, the galaxy presents a complex structure with both smooth and somewhat perturbed components.
