This galaxy presents as a spiral galaxy, viewed at an angle. It is estimated to be about 4.4 kpc in radius. A faint, diffuse disk surrounds a central bulge. The bulge appears moderately sized. Broad, loosely wound spiral arms are observed. The galaxy exhibits colors suggestive of active star formation within the arms. A bar-like structure may be present in the central region. There is no visual evidence of significant tidal disturbances or ongoing major mergers, although minor interactions cannot be ruled out. 
