The galaxy presents as a relatively faint, elongated structure. Its morphology indicates an edge-on disk galaxy. The disk appears thin and the bulge is not very prominent. There is some suggestion of minor internal structure or dust lanes within the disk. The galaxy exhibits a blueish hue, potentially indicating active star formation. No signs of major mergers or tidal disturbances are clearly visible, but there are slight irregularities in the disk that could suggest a minor interaction or internal instability. The galaxy appears relatively isolated in this field, with no obvious companion galaxies nearby.