The galaxy appears to be an elongated, edge-on spiral or lenticular galaxy. Its overall form is smooth with a noticeable central bulge that fades gradually into the galactic disk. The color distribution reveals a subtle gradient, suggesting variations in stellar populations. The central bulge exhibits a yellowish-white hue, potentially indicating older, redder stars. Moving outwards from the center, hints of blueish tones are observed, possibly indicative of younger, hotter stars within the galactic disk. There is no sign of major disturbances due to merging or tidal interactions.