This galaxy appears to be a disk galaxy, likely seen at a high inclination. The central bulge is elongated and relatively bright, exhibiting a smoother light profile compared to the faint disk. There are hints of structure within the disk, suggesting the presence of spiral arms, though the resolution limits a clear identification. There might be some interaction or merger event occurring, as suggested by the overall shape of the disk which is slightly disturbed, but this cannot be definitively stated based on the image alone. The blue color suggests that the galaxy has recent star formation, which is occurring throughout the galaxy, most prominently within the disk. The overall color is dominated by light at shorter wavelengths. The galaxy has a central concentration of older stars, and the disk appears to have some dust lanes. The overall luminosity indicates a moderate size for this galaxy compared to other galaxies at a similar distance.
