The galaxy appears to be relatively compact and centrally concentrated. It has a somewhat irregular morphology, lacking a clearly defined spiral structure or elliptical shape. There are indications of possible disturbances or tidal features in the outer regions of the galaxy, particularly a faint extension of material on the south side. The central region is bright, suggesting a significant concentration of stars and/or active galactic nucleus activity. Color variations are present, with the central region appearing predominantly blue-white, possibly indicating recent star formation, while the outer regions show a more greenish hue. Overall, the galaxy exhibits characteristics that could be indicative of an ongoing or recent merger event, or some form of significant gravitational interaction with another galaxy.
