The galaxy appears to be undergoing a significant interaction or merger event. The primary component exhibits a relatively smooth, somewhat spherical morphology, potentially indicative of an elliptical galaxy or a bulge-dominated system. However, the overall structure is highly irregular, with several distinct luminous knots and extended tidal features. A possible tail-like structure emanates from the main body, suggesting gravitational disruption. The color gradient transitions from redder hues in the central regions to bluer tinges in the outer extensions, which may imply differing stellar populations. There is evidence of ongoing or recent star formation within the disturbed regions.
