This galaxy presents an ambiguous morphology, appearing neither purely elliptical nor exhibiting a well-defined spiral structure. It appears to be undergoing a significant interaction or merger, as evidenced by the asymmetric distribution of light and the presence of what might be tidal features. The primary body of the galaxy is elongated, suggesting a possible ongoing collision. The color gradient is subtle, with a tendency towards redder hues in the core and a slightly bluer tint in the faint outskirts, indicative of some degree of star formation, although it appears to be relatively subdued. The overall profile seems rather smooth, but the disturbances are noticeable, suggesting that the merger is in an advanced stage.
