This galaxy exhibits a complex morphology, presenting characteristics of both smooth and featured structures. The central region is dominated by a bright, relatively smooth and concentrated luminosity profile, possibly indicative of an older stellar population or a bulge component. Extending outwards, there are hints of a disk-like structure, though it appears to be significantly perturbed or undergoing interaction.

Evidence of disruption is visible in the form of asymmetric light distribution and possible tidal features or distortions. One distinct region shows a bluer color, suggesting ongoing star formation. This localized star formation could be triggered by gravitational interactions. The overall color gradient suggests a mix of stellar populations with varying ages. The relatively small angular size of the galaxy on the image indicates that it is likely a distant object.
