The galaxy presents as a lenticular or edge-on spiral, characterized by a smooth, elongated profile. A discernible central bulge exhibits a yellowish-orange hue, suggesting an older stellar population and reduced recent star formation activity. The outer disk appears bluish, indicative of younger, hotter stars, although this region is not sharply defined, lending to the galaxy's smooth appearance. The galaxy’s shape is markedly elongated, approximately 8.7 kpc in effective radius, with a high degree of oblateness. There is no obvious indication of strong spiral arm structures or a prominent dust lane; however, the galaxy's inclination complicates detailed morphological assessment. No obvious signs of recent major merger activity are visible, however minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively massive system, with ongoing, albeit potentially low, levels of star formation.
