The galaxy exhibits a disturbed morphology, potentially indicating an ongoing or recent interaction. There is evidence of a distorted disk structure with faint, diffuse arms extending outward from a central bulge. The bulge region appears relatively smooth and concentrated. Star formation appears to be active within the arms, indicated by regions of bluer light, while the central bulge exhibits yellower hues possibly suggestive of an older stellar population. There is a faint tidal tail-like structure extending from one side of the galaxy suggesting interaction with another galactic body. Overall, the galaxy appears to be in a dynamic state.
