The galaxy presents with a somewhat disturbed morphology, displaying features suggestive of a recent or ongoing interaction. A central, relatively bright, and somewhat smooth component is apparent. This region exhibits a concentrated luminosity. Fainter extended structures emanate from this central zone, indicative of possible tidal features or distorted spiral arms. The galaxy exhibits color gradients, transitioning from bluer hues at the outermost edges to redder tones closer to the core, potentially suggesting differential stellar populations. Overall, the system appears to be in a non-equilibrium state, showing signs of dynamical activity, although there is no indication of a major merger.
