The galaxy appears to be undergoing a significant interaction, potentially a merger with another galaxy or a period of tidal disturbance. The primary body of the galaxy is relatively smooth and elliptical in shape, with a concentrated central bulge region. A secondary component, distinct in color and morphology, is visible to one side, suggesting an ongoing interaction. This secondary component exhibits bluer colors, possibly indicative of younger stellar populations or enhanced star formation activity. There is a streamer or tail like artifact that trails away from the primary body, possibly representing a tidal tail formed during the interaction. Dust lanes or other obscuring features are not readily apparent, though the overall color gradient suggests a complex internal structure.
