The galaxy appears as a luminous object, with a smooth, concentrated core. The primary color observed is a yellow-red hue suggesting an older stellar population dominating the galaxy's composition. The overall structure appears somewhat elliptical, with a high degree of central concentration and a slight extension along one axis. Evidence suggests that it is likely undergoing, or recently underwent a significant merger or tidal interaction with another galaxy. This is based on the disrupted morphology and the hint of a tidal tail extending from the main galactic body. Star formation rate is relatively low within the galaxy. Overall, the system appears to be an evolved galaxy, potentially a product of galactic mergers.
