The observed galaxy appears as an elongated, lenticular or spiral system viewed edge-on. A distinct central bulge is visible, appearing yellowish in color, indicative of an older stellar population. The galactic disk, extending outwards from the bulge, appears relatively smooth and featureless, showing limited evidence of distinct spiral arms. Dust obscuration is potentially present along the galactic plane, visible as a dark band bisecting the galaxy. There is no indication of recent major merger events or significant tidal disturbances. The galaxy's colors suggest moderate star formation activity.
