This galaxy presents a disturbed morphology, potentially indicative of an ongoing or recent merger event. A prominent central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars. Extending outward from this central region are faint, diffuse features. There is a clear asymmetry in the outer structures, with one side appearing more elongated than the other. Irregularities are observed in the form of clumpy regions within the galaxy, and a tidal tail emanating from the main body. Color gradients are present across the galaxy; the central region shows redder hues, possibly indicating an older stellar population, while the outskirts have bluer tones, which could be a signature of ongoing star formation. These morphological characteristics, combined with the observed color variations, strongly suggest the galaxy is undergoing some form of interaction. 
