The object appears to be a spiral galaxy, seen nearly edge-on. There is a prominent central bulge, appearing smooth and concentrated. The disk component is visible as a faint, elongated structure extending outwards from the bulge. The bulge appears more yellow/orange in color than the rest of the galaxy, which may be due to an older stellar population. Evidence of a disk suggests the galaxy is likely actively forming stars, though at a relatively low rate. The overall structure of the galaxy appears mostly undisturbed, with no obvious signs of a major ongoing merger, although there may be minor irregular features, indicating a past or ongoing minor interaction with another galaxy.
