The galaxy presents as a relatively compact object with a disk-like structure seen nearly edge-on. A prominent dust lane bisects the galaxy, obscuring the central regions. The core exhibits a bright, concentrated light profile, suggesting the presence of either a dense stellar population or an active galactic nucleus. The disk itself appears to be relatively smooth and featureless. Weak evidence of spiral arms or other detailed structures within the disk. Faint extended emission surrounds the central region, possibly indicative of a halo or tidal features. There is a slight asymmetry in the galaxy's light distribution.
