The galaxy presents as a relatively small, faint, and somewhat elongated structure. Its overall color appears bluish, suggesting a younger stellar population or ongoing star formation. There is a subtle central concentration of light, implying the presence of a bulge or a more densely populated central region. The galaxy lacks a clear spiral arm structure, and appears rather amorphous or lenticular. There are no apparent major disturbances or signs of an ongoing merger, although there are slight irregularities within the disk. The smoothness of the galaxy's light distribution indicates a relatively evolved system, potentially transitioning from a spiral to a more quiescent state.
