The galaxy presents an overall disk-like morphology, viewed at a high inclination angle, close to edge-on. A distinct central bulge is visible, appearing brighter and more concentrated than the outer regions of the disk. The disk itself exhibits a complex structure, with some evidence of internal features. A ring-like structure may be present around the bulge. The galaxy's color profile indicates a central concentration of bluer light, particularly within the bulge and in a central band, suggesting ongoing star formation. Redder colors are observed in some regions of the ring. Some disturbance or distortion in the disk's structure is hinted at, possibly indicative of minor tidal interactions or internal dynamical processes. The overall impression is of a spiral galaxy with a prominent bulge, ongoing star formation, and a complex internal structure.
