The galaxy presents as an edge-on or highly inclined spiral, exhibiting a flattened, disk-like structure. A central bulge is visible, characterized by a concentrated, yellowish-white luminosity, suggesting a population of older stars. Fainter, diffuse bluish-white light emanates from the galactic disk, indicative of younger stellar populations and potential star-forming regions. The galaxy's overall morphology appears relatively smooth, with no prominent signs of ongoing major mergers or tidal disturbances. There are hints of dust lanes along the galactic plane, obscuring some of the background light. The galaxy appears elongated, showing a significant difference between its major and minor axes.
