The galaxy presents a distinct edge-on morphology. A prominent bulge dominates the central region, exhibiting a smooth and rounded structure. The surrounding disk appears thin and elongated, oriented nearly along our line of sight. Dust lanes may be present within the disk, though this is difficult to ascertain with certainty given the image resolution and viewing angle. The galaxy exhibits a colour gradient, with the central bulge appearing more yellowish, suggestive of an older stellar population, while the disk shows hints of bluer hues, potentially indicating ongoing star formation. There are no readily apparent signs of significant recent merger activity or major tidal disturbances based on visible asymmetries. The overall structure suggests a galaxy with a significant spheroidal component and a well-defined disk.