The galaxy presents a complex morphology, exhibiting characteristics of both smooth and disturbed structures. The central region displays a bright, concentrated core, suggesting a possible bulge component. The surrounding light appears diffuse and extended, with hints of a possible disk or tidal features. There is an indication of potential interaction or merging activity. The color profile shows a gradient from bluer colors in the fainter regions to redder colors near the center, which could suggest varying stellar populations or dust content. Faint redder areas suggest star forming regions that may have been disrupted by the interaction. Overall, the galaxy appears to be undergoing some form of evolutionary process, possibly driven by a gravitational interaction. Further analysis would be required to determine the exact nature and extent of this activity.
