The galaxy appears to be a spiral galaxy, viewed edge-on. A prominent dust lane bisects the galaxy horizontally, obscuring the central bulge. The bulge itself appears relatively large and centrally concentrated. The disk is elongated and appears thin. The galaxy exhibits little evidence of significant tidal disturbances or ongoing mergers. No obvious spiral arm structures or star-forming regions are directly visible. The bulge appears more rounded. The overall color suggests a slightly older stellar population.
