The galaxy presents as a disk galaxy, observed at an almost edge-on inclination relative to our line of sight. A distinct bulge is not clearly visible; it likely has a small bulge, or possibly a pseudo-bulge, given the disk's morphology. The dust lane appears prominent along the mid-plane. There is a noticeable bluer color profile distributed along the disk, suggesting the presence of ongoing star formation. Irregularities are present in the disk structure, indicating minor disturbances or tidal interactions. The galaxy exhibits a moderate to high redshift, suggesting a substantial distance. The galaxy does not appear to be undergoing a major merger; any interactions are minor and do not significantly disrupt the overall structure. 
