The galaxy presents a complex morphology, exhibiting features suggestive of both a smooth central component and a more disturbed or irregular outer structure. The central region is dominated by a bright, concentrated luminosity, appearing somewhat amorphous without a clearly defined nucleus. Diffuse light extends outwards from this core.

Asymmetrical features are apparent within the galaxy's structure, including subtle disturbances or distortions in the distribution of light. Patches of redder hues are evident, possibly indicative of dust lanes or regions of older stellar populations. Blue tinges are present also, possibly indicating areas of active star formation. The overall impression is of a galaxy undergoing some form of interaction or internal dynamic process that is disrupting its regular morphology. While a significant fraction of the galaxy's light appears smooth, clear disturbances are present, and are most likely the result of ongoing or recent gravitational interaction or a merger event.
