This galaxy appears to be undergoing a significant interaction or merger. The morphology is disturbed, displaying irregular features rather than a clear spiral or elliptical structure. The central region shows a concentration of light, but it is not a well-defined, smooth bulge. Instead, it is mottled and asymmetrical, with extensions or tidal tails faintly visible. There is no readily apparent disk component, and there are luminous knots distributed throughout the body. This suggests active star formation regions triggered by the interaction. Overall, this is a galaxy in a state of flux, likely the result of a past or ongoing gravitational interaction with another galaxy.
