The galaxy presents as an elongated, spindle-shaped structure. A prominent central bulge is evident, exhibiting a yellowish-orange hue suggesting an older stellar population. The disk, seen nearly edge-on, displays a bluer color, indicative of younger, hotter stars and ongoing star formation. There is some indication of minor disturbances in the disk, but no significant signs of a major merger are apparent. Overall the galaxy has a smooth morphology, although with some notable features within the disk.
