This galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent dust lane bisects the galaxy's length, obscuring the central bulge and contributing to a darker, more subdued appearance along the mid-plane. The bulge appears elongated and primarily consists of older stellar populations. Faint extensions of the disk can be observed on either side of the central plane. There is no apparent indication of current high star formation. There is no evidence of strong tidal interactions or major mergers based on visual inspection of the galaxy's structure, although faint wisps extending beyond the primary disk region cannot be ruled out. The overall morphology suggests a relatively settled and unperturbed state.
