The galaxy exhibits a moderately disturbed morphology, with a disk-like structure that appears slightly warped or perturbed. There is a hint of possible tidal features or minor disturbances, suggesting a potential past or ongoing interaction or merger event. The main body of the galaxy is slightly elongated, which could be due to the interaction or an intrinsic bar structure. The color distribution indicates the presence of both older stellar populations, indicated by the reddish hues, and regions of active star formation, which appear bluer. The galaxy's light distribution is somewhat irregular and not entirely smooth, further supporting the presence of some internal structural features.
