This galaxy exhibits a complex morphology, indicative of an ongoing interaction or merger. A central, somewhat diffuse region is present, surrounded by more distinct features. To the northeast, a prominent, reddish component is observed, suggesting a region of older stellar populations or significant dust obscuration. To the west, a more elongated, yellowish structure extends outward, possibly a tidal tail or a disrupted arm resulting from gravitational interactions. The central region displays a bluer hue, indicative of the presence of younger, hotter stars. Overall, the galaxy's structure deviates significantly from a regular elliptical or spiral form, strongly suggesting it is in a dynamic state of merging with another galaxy or experiencing significant internal disturbances.
