The object appears to be a spiral galaxy viewed edge-on. A central bulge is visible as a concentration of light, with a disk extending outwards on either side. The bulge appears relatively smooth. The disk exhibits some degree of clumpy structure but shows no obvious spiral arm features from this perspective. There appears to be more light emitting from one end of the galaxy than the other, suggesting asymmetry. The galaxy is primarily blue, with a slight reddening toward the central bulge, suggesting a younger stellar population throughout the galaxy. This also suggests ongoing star formation within the disk. The overall morphology indicates a relatively low mass and a disk that is not well-defined, as indicated by the asymmetrical nature of the observed light and structure. There may be minor tidal disturbances or interactions, given the asymmetric distribution of light.
