The galaxy presents with an overall elongated morphology, approximated as a prolate spheroid. The luminosity profile exhibits a centrally concentrated, brighter region. This core exhibits a slightly redder hue. Extending outwards from this central region is a less luminous, more diffuse halo with a bluer color profile. The halo shows some evidence of possible disturbances in its structure. The overall shape hints towards a disk, with the brighter, redder central region acting as a bulge. There is also an indication that the object may have been a merger, due to its morphology. Overall, the object appears to be a single galaxy, with the possibility of minor interactions, though further study is needed to determine the full properties and history.
