This galaxy presents as a slightly elongated, disk-like structure. The overall color appears bluish-white, suggestive of a population of relatively young, hot stars. There is some evidence of faint, diffuse spiral arm structures emanating from the central region, although these are not sharply defined. The core of the galaxy appears brighter and more compact than the outer regions, possibly indicating a higher density of stars or the presence of a central bulge. The galaxy does not show any obvious signs of a major ongoing merger, although there may be some minor disturbances or irregularities in its structure. It is relatively small.
