The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent interaction. The main body displays a diffuse, somewhat irregular structure, lacking a clear spiral arm definition. There appear to be tidal features extending from the main body, specifically one extension towards the lower left side of the galaxy, with a concentrated light source within it. The primary body of the galaxy presents a bluer hue in its outer regions, possibly indicating ongoing star formation. Overall, the galaxy appears to be undergoing significant dynamical activity, suggesting a system that is not in equilibrium.
