The galaxy appears to be a mid-sized system with evidence of morphological disturbance. Its overall color profile suggests a fairly even distribution of stellar populations, with a slight bluing towards its outer regions. There are some faint features that indicate a possible ongoing interaction or recent merger event. A plume or tidal tail-like structure extends away from the primary body, possibly indicative of gravitational disruption. This could be from the merging of another smaller galaxy. While some areas look smooth, there is also some indication of clumpy structures with higher surface brightness, maybe from star forming regions or dust absorption. The core region shows a more condensed, smoother appearance with possibly some tidal features wrapping around it.
