The galaxy presents as an edge-on spiral, characterized by a prominent, bright central bulge. This bulge exhibits a smooth, rounded morphology and a yellowish hue, suggesting a population of older stars. A disk component is clearly visible, extending outwards from the central bulge on either side, and appears to be the dominant morphological feature. The disk demonstrates a complex structure with some indications of dust lanes or other features, giving a hint of a spiral structure. The galaxy shows no apparent signs of major mergers or significant tidal disturbances, appearing relatively undisturbed. The red shift indicates that it is far away, so appears quite small.