The galaxy appears to be a spiral galaxy, viewed at an oblique angle to our line of sight. There is a central bulge which exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge, we observe a fainter, bluer disk, indicative of ongoing star formation. The disk appears elongated, further supporting the angled perspective. There is some irregularity in the disk structure, but no major disturbances or clear signs of a major merger event are visible. The apparent axis ratio suggests a cigar-like shape. The galaxy is relatively compact. There is likely a degree of smoothness to the overall light distribution, but some features in the disk suggest that this could be a spiral galaxy.
