The galaxy presents as a relatively compact object with a slightly elongated, irregular morphology. The central region exhibits a bright, concentrated luminosity, suggestive of a substantial stellar population or possibly an active galactic nucleus, though no distinct point source is readily apparent. The overall color appears bluish, particularly in the diffuse halo surrounding the core, which indicates the presence of younger, hotter stars and recent star formation activity. Some minor disturbances appear to be present in the morphology, with asymmetries or tidal features possibly indicating interaction or a minor merger. The overall structure indicates a classification somewhere between a smooth elliptical and a disk galaxy with some notable features or disturbances.
