The galaxy presents as a faint, elongated lenticular form, likely a spiral galaxy viewed edge-on. A subtle central bulge is visible, with a slight boxy appearance. The dust lane bisects the galaxy’s disk, obscuring light from the galactic plane and indicating a significant amount of interstellar dust. The galaxy appears relatively undisturbed, lacking significant signs of recent or ongoing major mergers. There is a slight blueish tint, suggesting a degree of active star formation. The size of the galaxy is approximately 8 kiloparsecs across, implying that this is a dwarf galaxy.
