The galaxy presents with an overall elongated morphology. The core region displays a higher concentration of light, appearing more luminous than the surrounding regions. There is evidence of asymmetry in the light distribution extending from the core, with what appears to be tidal features or a disturbed morphology indicating a potential interaction or merger. A plume-like structure extends from the main body. The color gradient suggests a shift in stellar populations or dust content across the galaxy, with a bluer hue present in the extended structures compared to the yellower core. The overall structure suggests a galaxy undergoing some form of gravitational disturbance.
