The object presents as a spiral galaxy, observed at an oblique angle relative to its galactic plane. The central bulge is a prominent feature, exhibiting a moderate concentration of light, surrounded by a slightly less concentrated disk. Faint, tightly wound spiral arms appear to emanate from the central region. The overall color of the disk is bluish, suggesting a relatively young stellar population and ongoing star formation. There are no obvious signs of a strong bar structure bisecting the bulge. Visual evidence suggests a galaxy undergoing active star formation, but with no major merging activity readily apparent. 
