The galaxy appears to be a spiral galaxy seen nearly edge-on. A prominent central bulge exhibits a yellow-orange hue, indicating a population of older stars. The disk is visible as a flattened structure extending outwards from the bulge, with hints of bluish light suggesting the presence of younger, hotter stars. A dark dust lane is suspected along the midplane of the disk, obscuring some of the light from the bulge and disk regions, but this is uncertain due to low spatial resolution. The overall morphology suggests that the galaxy is actively forming stars, although at a relatively low specific rate. There may be minor disturbances to the outer disk, but no major ongoing mergers are apparent. The galaxy does not have a completely smooth appearance, with some signs of faint, irregular structure within the disk.
