The galaxy appears as a highly inclined disk galaxy, observed nearly edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge and providing a strong indication of a flattened disk structure. The central region of the galaxy exhibits a yellowish hue, suggestive of an older stellar population. The outer regions display a bluer color, hinting at the presence of ongoing star formation. There is no evidence of significant tidal features or major mergers, though some minor disturbances may be present. The overall morphology is suggestive of a relatively undisturbed, though perhaps slightly perturbed, spiral galaxy.
