The galaxy presents with a disk-like morphology, albeit with significant disturbances in its structure. There is evidence of a tidal tail emanating from one side, suggesting a possible interaction with another galaxy or recent merger event. The central bulge region is not well-defined, exhibiting a diffuse and asymmetric distribution of light. Star formation appears to be occurring at a moderate rate, indicated by the presence of localized regions of bluer light, although redder light overall indicates older stars. Dust lanes are visible, obscuring parts of the disk and contributing to the galaxy's complex appearance. Overall, the galaxy exhibits characteristics of a dynamically active system.
