The galaxy presents a somewhat disturbed morphology. It appears to be in the process of merging with another galactic body. A primary, larger component exhibits a smooth, elliptical profile, with a predominantly yellow-red hue, indicative of an older stellar population and potentially a lower rate of on-going star formation. Evidence suggests a mass of about 10^10 solar masses. A secondary component shows a higher degree of blue tint suggesting a younger stellar population and higher star formation rate, appears to be interacting with the primary galaxy, causing tidal disturbances. It has an irregular, asymmetrical shape, suggesting a disruptive gravitational interaction. There are some faint possible tidal features extending away from the main body of the interacting system. The overall system is relatively compact.
