The galaxy presents as a disk galaxy, viewed at an oblique angle, exhibiting a flattened, elliptical profile. A notable central bulge is present, appearing as a bright, concentrated region. The disk component displays a mottled texture, suggestive of spiral arm structures, although they are not sharply defined. The overall color of the galaxy is generally blue, with the bulge area displaying a whiter hue, potentially indicating a difference in stellar populations. There are no obvious signs of a major ongoing merger, although some minor disturbances cannot be ruled out at this resolution. The disk appears to be significantly larger than the bulge, which is less than a third the size of the visible disk. 
